The galaxy presents as a centrally concentrated, largely featureless, and rounded system. It exhibits a smooth, elliptical morphology with minimal discernible structure within the observed photometric bands. The core region is characterized by a bright, yellowish hue, suggestive of an older stellar population. This core gradually transitions into a fainter, bluish halo. This halo suggests the presence of a more dispersed population of stars and potentially some ongoing, albeit limited, star formation activity. There is no apparent evidence of a prominent disk structure, spiral arms, or significant dust lanes. The overall appearance indicates a galaxy that is likely in a relatively quiescent state, not undergoing any major merger events or experiencing intense starburst activity. There is a subtle indication of minor disturbance, perhaps the result of a previous interaction with another system.
