The galaxy presents an elliptical morphology, displaying a smooth, featureless appearance with a high degree of central concentration. The light profile suggests an older stellar population, particularly towards the core, indicated by the redder hues. The galaxy exhibits a slight elongation, appearing as an ellipse rather than a perfect sphere. There are no distinct spiral arms or prominent dust lanes visible. The object seems relatively undisturbed, with no obvious signs of recent mergers or major interactions. A subtle color gradient is observed, with the central region appearing yellower and the outer regions becoming slightly bluer. The galaxy's overall structure indicates a relatively quiescent state, consistent with a system dominated by older stars with a moderate star formation rate.
