This galaxy exhibits a morphology that appears largely smooth and elliptical. The central region presents a concentrated luminosity, suggesting a prominent galactic nucleus. Moving outward from the core, the light gradually decreases. The shape is mostly round. The color distribution suggests a population of older stars. There does not appear to be a strong presence of dust lanes or spiral arm structures. There is no indication of any ongoing major merger activity or significant tidal disturbances affecting the galaxy's structure. Overall, it looks like a relaxed system. 
