The galaxy presents as a relatively smooth, centrally concentrated object. Its overall morphology appears elliptical. The central region exhibits a bright, yellowish-white core, suggestive of an older stellar population. Moving outwards from the center, the galaxy transitions to a fainter, more diffuse halo with a subtle reddish tint, possibly indicating the presence of dust or a population of older, redder stars. There is no obvious spiral structure or prominent disk. There's no evidence of any major ongoing merging events or strong tidal disturbances. Minor asymmetries may be present, but they are not pronounced.
