The galaxy presents as a relatively smooth, centrally concentrated object. It has an elliptical morphology with a high degree of roundness, though a slight elongation is detectable. The galaxy exhibits a bright, concentrated core region that gradually fades towards the outer edges. No distinct spiral arms or bar structures are apparent. The light distribution suggests a smooth transition from the central bulge outwards. The color appears generally uniform across the galaxy, indicating a possibly older stellar population. There is no evidence of any major ongoing merger activity or significant tidal disturbances in the image. Minor irregularities along the outskirts may suggest minor interactions or accretion events in the galaxy's past.
