The galaxy appears to be a relatively smooth, elliptical system. The central bulge region exhibits a bright, concentrated luminosity, suggesting a high density of stars. The overall shape is somewhat elongated, showing slight deviation from a perfectly circular morphology. Faint, diffuse features extend outwards from the core, potentially indicating a faint disk component or tidal disturbances. The galaxy displays a color gradient, with the central region appearing more yellow-white and the outer regions exhibiting a slightly bluer hue, suggestive of possible ongoing, but low, star formation in the outer areas. No obvious spiral arms or dust lanes are discernible in this image. Evidence suggests the galaxy has experienced some gravitational interaction, although it does not appear to be a major ongoing merger.
