The galaxy presents as an elliptical morphology, exhibiting a smooth and centrally concentrated luminosity profile. The core region is significantly brighter and appears almost spheroidal, with a gradual decrease in intensity outwards.  There is little to no evidence of spiral arm structures or prominent dust lanes, indicative of a relatively quiescent system. The overall color is generally yellowish, suggesting a stellar population dominated by older, redder stars.  There is a very slight elongation of the galaxy, but it is close to spherical.  Faint, diffuse extensions are possibly visible, indicative of a stellar halo.  There is no noticeable interaction with neighboring galaxies or signs of major disturbances.
