The galaxy presents as a fairly concentrated, luminous object. It appears elliptical in shape, with a smooth, relatively featureless profile. The central bulge exhibits a high degree of luminosity, suggesting a concentration of older stellar populations. Moving outwards, the galaxy gradually fades into a less defined halo. There is a slight elongation that is barely visible. Based on the lack of discernible spiral arms or dust lanes, it can be classified as an early-type galaxy. The galaxy shows a redder color. There is no apparent indication of ongoing major merger activity or significant tidal disturbances. The overall morphology suggests a relatively evolved system.
