The observed galaxy presents as a spiral galaxy with a relatively well-defined structure. Its morphology indicates a prominent disk component viewed at a moderate angle, not quite face-on, but not significantly edge-on either. The spiral arms appear tightly wound, tracing a well-defined pattern that extends outward from the central region. These spiral arms are multi-armed, branching from the central core with areas of increased luminosity along the arms, suggesting active regions of star formation. A moderate bulge is visible at the galaxy's center, though not overwhelmingly dominant. The central bulge has a smoother texture and a yellowish hue, indicating an older stellar population. There is no clear visual evidence of a strong bar structure, although subtle indications might be present. The overall color profile suggests a mix of stellar populations, with bluer hues concentrated along the spiral arms and a more redshifted central bulge. There are no immediate signs of a major merging event, though some subtle asymmetry or minor disturbances might be present upon closer inspection, consistent with the appearance of past or ongoing interactions with nearby galaxies.
