This galaxy presents a largely elliptical morphology, exhibiting a smooth light distribution with no apparent spiral arm structure or significant dust lanes. The galaxy's light is centrally concentrated, with brightness decreasing gradually towards the outer regions. Color gradients are subtle, with the core appearing slightly yellower and the outer regions tending toward a bluer hue. There is no sign of ongoing major mergers or tidal disturbances. The galaxy has a moderately compact size, considering its distance, and it appears to be a well-defined, relatively evolved system with signs of current star formation activity.
