The galaxy presents as a roughly circular, unresolved object. It appears to be primarily smooth in texture. Its central region exhibits a higher luminosity than the surrounding area, suggesting a concentration of stars or active galactic nucleus. Subtle irregularities in the isophotes are present, potentially indicating minor disturbances in its structure, however these are not major disruptions. The color profile suggests a population of older stars, as evidenced by the redder hue. No distinct spiral arms or a prominent disk component is evident.
