The galaxy presents a relatively smooth, elliptical morphology. There is minimal evidence of spiral arm structures or a prominent disk. The light distribution appears highly concentrated towards the center, with a rapid decrease in intensity towards the outer regions. The galaxy exhibits a generally round shape, with slight deviations that may indicate minor tidal interactions or internal asymmetries. There is no indication of a major ongoing merger, although the possibility of past mergers cannot be ruled out. The color profile indicates a stellar population that is largely composed of older stars.
