The galaxy presents an overall elliptical morphology, appearing mostly smooth. The central region exhibits a concentration of light, suggestive of a bulge. Extending outwards from the central bulge is a slight asymmetry, possibly indicating a weak disk-like structure or tidal interactions. There is no significant spiral structure apparent. The color profile indicates a redder hue in the central regions, potentially indicative of an older stellar population, while fainter blueish colors are evident around the periphery. The overall shape hints at a possible recent minor merger event or disturbance, although it does not dominate the overall appearance of the galaxy. Based on its absolute magnitudes and mass estimates, this is a massive galaxy, but with a fairly low star formation rate.