The galaxy appears to be a relatively smooth, elliptical-like object with a concentrated central bulge. The light distribution is generally centrally concentrated, with a gradual falloff in intensity towards the edges. The galaxy exhibits a faint, diffuse halo surrounding the main body. There is a hint of a possible disk structure, but it is not clearly defined. The color is primarily a blend of yellowish and reddish hues in the central region, which is indicative of an older stellar population, with slightly bluer tones present at the periphery which may suggest more recent star formation. No prominent dust lanes or spiral arm structures are discernible. The overall morphology suggests the galaxy is undisturbed, without any major signs of ongoing mergers or interactions.
