The galaxy presents as a centrally concentrated, luminous object. Its morphology appears largely smooth, with a generally elliptical shape. There is a slight elongation discernible, though the galaxy is predominantly round. No distinct spiral arms or bar structures are readily apparent. Minor disturbances may be occurring within the galaxy, potentially small tidal interactions, but the main structure does not present any signs of a major merger. The central region appears bright and slightly more yellow in color compared to the outer edges, perhaps indicating an older stellar population concentrated in the core. Fainter, bluer regions may exist in the outer disk, indicative of younger star formation.