The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated, bright central region, suggesting a prominent bulge. The overall color appears to be a yellowish-white, transitioning to bluer hues in the outer regions. This color gradient may indicate a higher proportion of older stars in the core, with younger, bluer stars in the surrounding areas, indicative of ongoing or recent star formation in the disk. Some level of disturbed morphology is seen. There might be some signs of minor tidal disturbances, but the galaxy otherwise presents with a settled morphology. The galaxy is relatively large.
