The galaxy appears to be a relatively smooth, elliptical-like galaxy with a concentrated central bulge and a diffuse halo. The galaxy exhibits a yellowish-orange hue, suggesting a stellar population dominated by older, redder stars. There is no apparent structure, such as spiral arms or dust lanes, visible in the image, indicating it is likely a later type galaxy. Overall the galaxy appears fairly round and the light is distributed evenly. No major disturbances or tidal features are seen around the galaxy, hinting at a lack of recent major merger activity. It has a substantial stellar mass and a moderate star formation rate.
