The galaxy presents a relatively smooth morphology, appearing as a concentrated spheroid. The light profile increases steadily towards the center, culminating in a bright, somewhat diffuse core. The galaxy exhibits an elliptical shape, with a clear major and minor axis. The light distribution follows a de Vaucouleurs profile, with a high Sersic index value. The galaxy is generally red in color, possibly indicating an older stellar population and a lower rate of recent star formation. There may be some very subtle disk features, but they are not immediately obvious. There is no strong evidence of significant dust lanes or tidal disturbances.
