The galaxy presents as a centrally concentrated object with a predominantly smooth morphology. The light profile appears relatively featureless, lacking any distinct spiral arm structures or prominent dust lanes. The central region exhibits a yellowish-orange hue, suggesting a population of older stars. The galaxy's overall shape is somewhat elliptical, although there is some deviation from perfect roundness. There is no obvious indication of an ongoing major merger or significant tidal disruption. The galaxy appears relatively isolated, although faint hints of possible minor disturbances are present in the outer regions. The size of the galaxy is compact.
