The galaxy presents as a relatively smooth, elliptical-like structure with a slight elongation. The central region exhibits a concentrated luminosity, appearing nearly featureless and consistent with a bulge component. The color profile suggests a population of older stars, contributing to the galaxy's redder hue. Some bluer light is present in the outer regions, indicating a small amount of star formation. The galaxy does not display any strong indications of spiral arms or significant disturbances due to mergers. Its overall morphology is consistent with an early-type galaxy, likely an elliptical.
