The galaxy presents as an elliptical morphology, exhibiting a smooth and relatively featureless structure. The light is centrally concentrated, with a luminous core that gradually fades into the outer regions. The isophotes appear to be generally elliptical, with a moderate degree of ellipticity. The color profile suggests a population of older stars, as indicated by the yellow-red hue, especially within the central bulge. There is a subtle hint of a disk-like structure, although no spiral arms or significant dust lanes are visible. The overall appearance indicates a galaxy that is likely in a relatively quiescent state, with little ongoing star formation. There may be some minor disturbance present which is most likely the result of interactions with smaller satellite galaxies.
