The galaxy presents as a fairly symmetrical, elliptical-like structure with a smooth, diffuse appearance. Its color is predominantly yellowish-orange, suggesting an older stellar population and a lack of significant recent star formation. There is no discernible spiral arm structure or dust lanes visible in this image. The light is concentrated towards the center, indicating a central bulge. There is no evidence of tidal tails or strong distortions, which implies it is likely not undergoing a major merger. There appears to be a low level of star formation activity occurring within it, but the specific star formation rate is low. The galaxy appears relatively isolated, without any close companions. Its estimated size suggests that it is a relatively large galaxy.
