The galaxy presents a generally smooth, elongated profile, suggesting an elliptical morphology or possibly a highly inclined disk galaxy. The central region exhibits a bright, concentrated core indicative of a substantial stellar population or active galactic nucleus. A fainter, more diffuse component extends outwards from the core. Color gradients are subtle, but a slight reddening towards the center might indicate an older stellar population in the bulge, while bluer hues in the outer regions could suggest ongoing star formation. There is an apparent companion or tidal feature that is slightly bluer in color to the side of the center of the galaxy. Evidence for significant dust lanes or spiral arm structure is absent from this image. The galaxy's overall appearance is consistent with a system undergoing some form of interaction or past merger event, given its somewhat distorted shape and possible companion galaxy.
