The galaxy presents a largely smooth, elliptical morphology. The light distribution appears centrally concentrated with a gradual decline in intensity towards the edges. There is a very slight elongation, deviating minimally from a perfectly circular shape. The color gradient suggests a population of older stars, with a yellow hue dominating, potentially indicating a lack of significant ongoing star formation. There is no clear evidence of spiral arms, dust lanes, or other distinct features typically associated with disk galaxies. The general appearance indicates it is a relatively quiescent system without major ongoing merging activity or recent disturbances.
