The galaxy presents as a flattened, disk-like structure, viewed at a moderate inclination. It exhibits a central bulge that appears more concentrated and luminous, possibly indicative of a supermassive black hole. The bulge emits light on the redder end of the spectrum, perhaps signifying an older stellar population within that region. The disk surrounding the bulge is characterized by a bluer hue, which implies the presence of younger, hotter stars, and possibly ongoing star formation. The disk displays some irregularities, which may indicate recent or ongoing interactions with other galaxies. The edges of the disk are somewhat diffuse, with no sharply defined boundaries. Overall, the galaxy exhibits a morphology somewhere between elliptical and spiral, possibly a lenticular galaxy. There is a very faint hint of arms, but they are too faint to be able to characterize well.
