The galaxy presents an overall elliptical morphology, appearing largely smooth and well-defined. The light profile is concentrated toward the center, indicating a prominent bulge component. It has a relatively high luminosity, suggesting a considerable mass. The color is on the redder end, indicating an older stellar population and lower levels of current star formation. There is no distinct spiral arm structure or prominent dust lanes that can be observed. There might be some minor disturbances, suggesting that the galaxy could be undergoing some form of interaction with its surroundings, but this is inconclusive. The light distribution is consistent with a relaxed system and has an overall round shape. The galaxy does not appear to be undergoing a major merger.
