The galaxy presents an elliptical morphology, appearing as a somewhat elongated spheroid. It exhibits a relatively smooth light distribution with no apparent spiral arm structures or prominent dust lanes. The core region appears brighter and more concentrated than the outer regions, suggesting a higher density of stars towards the center. There is a slight color gradient, with the central region exhibiting a slightly yellower or redder hue compared to the more bluish outer halo, possibly indicating an older stellar population in the core. The galaxy shows no signs of major mergers or significant tidal disturbances in its immediate vicinity. The object appears relatively isolated within the observed field.
