The galaxy appears as a diffuse, centrally concentrated object with a generally smooth morphology. There is a slight elongation, but overall, it is moderately rounded. The central region exhibits a higher surface brightness, gradually fading outwards. No distinct spiral arms or bar structures are discernible. There are some subtle disturbances, which might suggest ongoing or past minor interactions with satellite galaxies. The galaxy appears to have a low rate of star formation. The overall color is consistent with an older stellar population, and it is a fairly massive galaxy.
