The galaxy appears to be a relatively compact and luminous object, exhibiting a generally elliptical morphology. The light is concentrated towards the center, suggesting the presence of a significant bulge component. The galaxy appears largely smooth in texture, with minimal visible substructure or distinct spiral arms. The color gradient is relatively subtle, tending towards redder hues which suggest an older stellar population. There are no obvious signs of ongoing major mergers or tidal disturbances, and it's roundish in shape. Based on the observed properties, this galaxy is likely a massive early-type galaxy with a relatively low star formation rate.
