The galaxy presents as a fairly smooth, elliptical structure with a concentrated central bulge. Its overall color appears to be reddish, which suggests an older stellar population. There is no discernible spiral arm structure. The light distribution is centrally concentrated, with a gradual decrease in intensity towards the edges. The galaxy's shape is generally round, with no major distortions or tidal features visible. There is no strong evidence of active star formation, with the colors indicating that the overall star formation rate is low. The image suggests that the galaxy is relatively isolated, without signs of recent or ongoing major merger activity.
