The galaxy presents as a somewhat diffuse, centrally concentrated object. It exhibits a generally smooth morphology. The color profile suggests a mix of stellar populations; bluer tints are observed within the central region, possibly indicating ongoing star formation, though the overall galaxy color leans towards redder hues, more typical of older stellar populations. There are slight asymmetries or disturbances in the outer regions, potentially signs of minor gravitational interactions or past merger events. The overall shape appears more elliptical than disk-like. The galaxy does not have a pronounced spiral structure.
