The galaxy presents as a disk galaxy, viewed at a moderate inclination. A central bulge is visible, appearing smooth and concentrated with a yellowish hue suggestive of an older stellar population. Surrounding the bulge is a fainter, bluer disk component. The blue color hints at ongoing star formation within the disk. The disk appears somewhat diffuse and lacks well-defined spiral arms, indicating a possibly flocculent or poorly defined spiral structure. The outer edges of the disk are not sharply defined, appearing more amorphous and indistinct. The overall morphology suggests a galaxy that is neither a pure elliptical nor a grand design spiral, but rather something intermediate, perhaps a lenticular galaxy or a loosely wound spiral galaxy with a prominent bulge and more diffuse, less structured disk. There may be evidence of minor interaction or tidal disturbances, although the asymmetry could arise from an active galactic nucleus.
