The galaxy presents a moderately elliptical morphology, appearing largely smooth and centralized. The light distribution is somewhat diffuse, with a color gradient suggestive of an aging stellar population. No distinct spiral arms or prominent dust lanes are discernible. The galaxy appears to exhibit signs of possible minor interactions or tidal disturbances, but it is also possible that it is in the process of merging with one or more galaxies. The central region is slightly brighter and redder than the outer regions.
