The galaxy appears to be a relatively smooth, centrally concentrated object. It exhibits an elliptical morphology with a high degree of roundness. The color profile suggests a significant population of older stars, with a general yellow-red hue. There is little to no evidence of spiral arm structures or significant dust lanes. The galaxy’s light is centrally condensed, forming a bright core that gradually fades into the outer regions. Based on its smooth appearance, it may be an elliptical galaxy with minimal ongoing star formation. There is also the possibility that it is a spiral galaxy seen face-on, where details of the disk structure may be obscured. There does not appear to be any ongoing merging activity or prominent tidal features.
