The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. There is a distinct lack of resolved spiral arm structures or prominent dust lanes. The central region exhibits a bright, concentrated luminosity profile, suggesting a significant stellar density and possibly a supermassive black hole actively accreting material, although no distinct active galactic nucleus features are apparent in this image.

The overall color appears yellowish-red, indicative of an older stellar population and potentially a lower rate of ongoing star formation. There is no clear evidence of any major merger events or significant tidal disturbances in the immediate vicinity of the galaxy, although subtle irregularities in the outer isophotes cannot be ruled out completely. The galaxy appears mostly quiescent.
