The galaxy presents as an elliptical morphology, characterized by a relatively smooth, diffuse light distribution. It exhibits a slightly elongated shape, deviating marginally from perfect circularity. The central region appears brighter and more concentrated, with a gradual decrease in luminosity towards the outer edges, indicating a density gradient. The galaxy's color profile suggests a population of older stars, with a redder hue dominating the central bulge and a bluer tint in the surrounding disc, possibly indicating a lower rate of star formation. There is a faint suggestion of internal structure or faint arms. Overall, the galaxy appears relatively undisturbed, with no obvious signs of recent mergers or major tidal interactions.
