The galaxy presents as a relatively smooth, elongated structure, consistent with an elliptical morphology. The light distribution suggests a centrally concentrated bulge, with a gradual decrease in luminosity extending outward. There is a color gradient apparent, with the core exhibiting a yellowish-red hue, potentially indicating an older stellar population, while the outer regions show a slightly bluer tinge, suggesting the presence of some younger stars. The lack of distinct spiral arms or prominent dust lanes supports its classification as an elliptical galaxy. There does not appear to be evidence of significant ongoing mergers or tidal disturbances based on the image. The overall symmetry and smooth light profile further reinforce this assessment. The apparent size is relatively compact.
