The galaxy presents as a largely smooth, elliptical morphology with a concentrated central bulge exhibiting a yellowish hue, suggestive of an older stellar population. The galaxy appears moderately luminous. There is a slight elongation to the galaxy's shape, though it mostly retains a rounded appearance. Minimal evidence of spiral arms or significant dust lanes is observed; any features of the like appear faint or otherwise lacking. There are no obvious signs of ongoing major mergers or strong tidal disturbances. The galaxy exhibits a colour gradient, with the central region appearing more yellow than the outer regions, which seem marginally bluer. This suggests a possible difference in stellar populations, with older stars dominating the core and relatively younger stars residing in the outer parts of the galaxy. Overall, it is a somewhat unremarkable galaxy, exhibiting standard elliptical characteristics.
