The galaxy presents a relatively smooth, elliptical morphology. The light distribution appears concentrated towards the center, with a gradual decrease in intensity towards the outer regions. There is little evidence of spiral arm structure or prominent dust lanes. The color is slightly red, suggesting an older stellar population with a low rate of ongoing star formation. There is no indication of a strong tidal interaction or recent merger event based on its morphology. Overall, the galaxy appears to be an evolved system, potentially a massive elliptical galaxy.
