The galaxy presents as a primarily smooth, elliptical-like structure with a concentrated central bulge. It exhibits a yellow-orange hue, suggesting an older stellar population with less ongoing star formation and a higher proportion of evolved stars. The overall shape appears mostly round, lacking any prominent spiral arms or disk-like features. There is no apparent sign of major mergers or significant tidal disturbances. The galaxy's light distribution is centrally concentrated, with a gradual decline in luminosity towards the outer regions. Based on its color and morphology, this galaxy likely represents a massive early-type galaxy that is no longer actively forming many stars.
