The galaxy presents a largely smooth, rounded morphology, indicative of an elliptical galaxy, or potentially a spiral galaxy seen face-on but with limited discernible spiral arm structure. Its overall color appears to be a yellowish-orange, suggesting a stellar population dominated by older, redder stars. A slight hint of blue or green is visible on its periphery, which could indicate regions of recent star formation.

The galaxy exhibits a centrally concentrated luminosity profile, gradually decreasing in intensity towards the outer regions. There is no evidence of strong tidal features or major disturbances in the galaxy's structure, which implies it is a relatively relaxed system. While some level of star formation may be present, the dominant stellar population and morphology suggest that this galaxy has a relatively low star formation rate.
