The galaxy presents as a spiral type, observed at a slight inclination. The central bulge appears relatively small and not distinctly prominent. Spiral arms are visible, exhibiting a loosely wound morphology. These arms are somewhat fragmented, containing areas of increased luminosity which may indicate active star formation regions. There are no distinct signs of a strong bar structure, but a faint, elongated structure can be seen through the center of the galaxy. The overall color suggests a mix of stellar populations, with bluer hues concentrated within the spiral arms and a more yellowish hue toward the central region. There is no evidence of major mergers or tidal disturbances in the immediate vicinity, though some minor irregularities in the arm structure may point to minor gravitational interactions. The galaxy's disk appears to be relatively thin.
