The galaxy presents as a centrally concentrated object with a generally smooth appearance. The central region exhibits a bright, yellowish-white core, indicating a high density of stars, possibly an older stellar population. Moving outwards from the core, the galaxy displays a diffuse, less luminous halo. The overall shape appears largely elliptical or spheroidal. There is little evidence of spiral arms or significant dust lanes. Subtle color gradients are observed, with the outer regions appearing slightly bluer compared to the core, potentially suggesting some ongoing star formation, although at a relatively low rate. There does not appear to be any major tidal disturbance or ongoing merger activity.
