The galaxy presents an overall smooth morphology, displaying a central bulge that appears nearly spherical, with a slight elongation along one axis. The light distribution suggests a concentration towards the core. The color profile exhibits a yellowish hue, which may indicate a population of older stars and a relatively low rate of ongoing star formation. There appears to be little to no evidence of prominent spiral arm structures or significant dust lanes. A minor tidal disturbance cannot be ruled out. Based on the morphology, a classification as an elliptical galaxy or a lenticular galaxy is plausible.
