The galaxy presents as a lenticular or early-type spiral, exhibiting a flattened, disk-like morphology. A prominent central bulge is observed with a bright, concentrated luminosity profile, possibly indicative of a supermassive black hole. Faint spiral arm structures or flocculent features may be present but not distinctly defined, suggesting that it could be an Sa galaxy.

The color gradient suggests an aging stellar population, with the central bulge appearing more yellow/red and the outer disk exhibiting a bluer hue, potentially due to younger stars or some ongoing star formation. However, the overall redder color implies a relatively low star formation rate. The shape of the galaxy is elliptical, with evidence of a bar which is not very prominent.

Dust lanes or significant obscuration are not easily apparent, consistent with a later stage of galaxy evolution where gas and dust have been largely consumed. The galaxy exhibits moderate inclination relative to our line of sight, allowing some structural details to be discernible.
