The galaxy presents as an elliptical morphology, elongated in shape. A concentrated central bulge of high luminosity is evident, exhibiting a yellowish hue, possibly indicating an older stellar population. The outer regions display a gradual decrease in luminosity and a subtle shift toward bluer colors, suggesting the presence of some younger stars. The overall structure appears smooth, with no obvious spiral arms or distinct dust lanes visible. There are no signs of any major mergers or significant tidal disturbances in its immediate vicinity, although subtle asymmetries could indicate minor interactions. The galaxy appears to be relatively isolated.
