The galaxy presents an elliptical morphology, appearing predominantly smooth in structure with a slight elongation. There appears to be some evidence of a possible interaction or minor disturbance, given the asymmetry in the light distribution. The galaxy's color gradient suggests a population of older stars dominating the central regions, exhibiting a redder hue. Conversely, areas with a bluer tint, possibly indicating on-going star formation. The observed features of the galaxy point towards a relatively evolved system.
