The galaxy presents a primarily smooth morphology, exhibiting characteristics of an elliptical or lenticular galaxy. The light distribution appears concentrated towards the center, with a gradual decrease in intensity as the radius increases. The overall shape is roughly circular, with a slight deviation suggesting a potential transition from a truly spherical morphology. There is little evidence of prominent spiral arms or significant dust lanes. The galaxy displays a relatively uniform color across its extent, with a somewhat yellowish hue. This suggests an older stellar population, typical of galaxies with lower rates of recent star formation. There are no readily apparent signs of major mergers or tidal disruptions. However, a minor disturbance could be present within the light profile, though not overtly distinct in the image.
