The galaxy appears as a roughly elliptical, smooth distribution of light. Its color is predominantly yellowish-orange, suggesting an older stellar population. The light is centrally concentrated, showing a bright core that gradually fades into the outer regions. There are no clearly defined spiral arms or dust lanes visible. The overall morphology indicates a galaxy that has likely undergone significant evolution, with little evidence of ongoing major star formation. There is no significant asymmetry or tidal features that would suggest it is in the process of merging.
