The galaxy presents as an elliptical morphology, appearing relatively smooth with no discernible spiral arm structure or prominent dust lanes. The light distribution suggests a centrally concentrated brightness profile, with a gradual decrease in intensity towards the outer edges of the galaxy. The core is bright and slightly orange, indicating a population of older stars. There are signs of distortion or tidal features, indicating possible past or ongoing interactions with other galaxies. The color suggests the presence of a more evolved stellar population. This galaxy appears to be a relatively massive system. Star formation is minimal based on the smooth appearance and color.
