The galaxy presents as a centrally concentrated, relatively smooth object. It has a generally elliptical shape, with the ratio of the major to minor axis appearing to be approximately 1.2:1. The luminosity profile increases steadily towards the center, where it reaches a bright, concentrated core. No distinct spiral arms or other pronounced features are discernible. There is a subtle bluing near the outer edges of the galaxy, which may indicate areas of more recent star formation, however the overall color is redder, suggesting an older stellar population is more dominant. There is a minor asymmetry, suggestive of a past or ongoing minor interaction, but the galaxy is mostly undisturbed.
