The galaxy presents as a concentrated, generally smooth object with an elliptical morphology, displaying a predominantly yellowish hue. The light distribution suggests a centrally concentrated structure with a gradual decrease in luminosity outward. The color indicates an older stellar population, with a relative paucity of ongoing star formation. There is no visible evidence of spiral arms or a distinct disk component. The galaxy is largely undisturbed, with no obvious signs of recent mergers or tidal interactions, maintaining a relatively round shape.
