The galaxy presents an overall smooth morphology, with a prominent, bright central bulge. The bulge exhibits a yellowish-white hue, indicative of an older stellar population. A disk component is present, extending outwards from the bulge, but is not sharply defined. The disk appears somewhat flattened and displays a bluer tint, suggesting the presence of younger, hotter stars and potential ongoing star formation. The galaxy's shape is elongated, with a moderate ellipticity; this galaxy would best be described as a lenticular type galaxy, as there seems to be no spiral structure. There are no obvious signs of significant tidal disturbances or ongoing merger activity, although there is some minor asymmetry. Overall, the galaxy appears relatively undisturbed and evolved.
