The galaxy presents as a relatively compact and moderately bright system. Its morphology appears to be primarily spheroidal, with a smooth overall appearance and a high degree of central concentration. There is some evidence of disturbance in its morphology, possibly indicating an interaction or merger event. Faint, diffuse tidal features or extended structures are weakly suggested, but could also be due to lower image resolution. The galaxy displays a color gradient, with a more yellowish or redder hue towards the central region, possibly indicative of an older stellar population. The outer regions appear slightly bluer, suggesting the presence of younger stars, or potentially ongoing star formation. It appears to be surrounded by a number of other objects.
