The galaxy presents as a largely smooth, elliptical or lenticular structure. A bright, concentrated central bulge dominates the morphology, with a yellowish-white hue suggestive of an older stellar population. The surrounding disk appears less defined, exhibiting a bluer color, which indicates a younger stellar population and possible ongoing, though potentially low-level, star formation. There may be faint and subtle spiral arm structures, but the image resolution does not allow for definitive identification. No major disturbances or tidal features are apparent; the galaxy appears relatively isolated and undisturbed. It is a single, mostly symmetric galaxy, without an obvious companion or merging partner.
