The galaxy appears to be elliptical in shape, displaying a smooth, concentrated central bulge that dominates its overall structure. There is a noticeable lack of distinct spiral arms or prominent dust lanes. The core of the galaxy exhibits a bright, yellowish hue, potentially indicating an older stellar population. Fainter, reddish areas are observed peripherally to the bulge, which may indicate regions of active star formation, although the star formation rate appears to be relatively low. There is slight asymmetry in its overall light distribution and some disturbances in the color of the halo, indicating possible interactions with another galaxy. The galaxy appears to be quite massive and relatively distant.
