The galaxy presents a distinct spiral structure, as evidenced by the faint, tightly wound arms extending from the central bulge. The arms exhibit a patchy, flocculent appearance, indicating active star formation regions. These regions appear blue, suggesting the presence of young, hot stars. The central bulge exhibits a yellowish hue, which is indicative of an older stellar population and a reduced rate of star formation. The galaxy does not show signs of significant interaction or merging with other galaxies, but displays some minor disturbances throughout. The overall shape appears somewhat elliptical, with a moderate inclination relative to our line of sight.
