The galaxy presents as a somewhat diffuse and elliptical object. The central region exhibits a higher concentration of light, fading towards the outer edges. The color appears generally yellowish-red, suggestive of an older stellar population. There is a slight hint of asymmetry in the light distribution, potentially indicating a minor gravitational interaction or internal disturbance. No distinct spiral arm structures or prominent dust lanes are discernible. Overall, the morphology is relatively smooth, lacking sharp or clearly defined features.
