The galaxy presents as a relatively smooth, elliptical-like structure. Its central region exhibits a concentrated luminosity, which gradually diminishes towards the outer edges. The galaxy's color appears to be on the redder end of the spectrum. There is a slight elongation, deviating somewhat from a perfect circle. No distinct spiral arms or prominent dust lanes are discernible within the galaxy's morphology. There are possible indications of minor disturbances, but the overall structure appears to be generally undisturbed, indicating it is not undergoing a major merging event.
