The galaxy presents as a smooth, elliptical-like structure, displaying a concentrated central bulge that transitions into a less dense halo. The light profile is relatively smooth, with no discernable spiral arms or bar structure evident. The color gradient shifts from a yellowish hue in the core, suggesting an older stellar population, to a bluish tint in the outer regions, indicative of ongoing, or recent, star formation activity. The overall morphology indicates that this galaxy may be in a relatively quiescent stage of evolution, although the bluer color in the outer regions implies a non-negligible rate of star formation. There may be some minor disturbances in the galaxy; however, there is no evidence of major mergers or significant tidal interactions. The galaxy displays a generally rounded form, with only a slight elongation along one axis.
