The galaxy presents a generally smooth, elliptical morphology. A bright, concentrated nucleus is observed, surrounded by a diffuse halo of lower surface brightness. The galaxy appears to be relatively isolated, with no obvious signs of major mergers or tidal disturbances. There is an absence of distinct spiral arm structures or prominent dust lanes. The overall color is indicative of an older stellar population, with a dominant yellow/red hue in the central regions. There are traces of bluer light suggesting some ongoing, though limited, star formation activity. The shape is approximately round, without significant elongation. Faint, diffuse features are visible extending outwards, which are likely part of the galaxy's outer halo.
