The galaxy presents a generally smooth morphology, appearing largely spheroidal in shape. The central region exhibits a concentration of light, suggesting a prominent galactic nucleus. The overall color profile is predominantly yellowish-white, possibly indicating a population of older stars. There is a subtle hint of a diffuse halo surrounding the main body of the galaxy. No distinct spiral arms or significant dust lanes are readily apparent, but there might be some minor signs of disturbance that are suggestive of past or ongoing interactions. The galaxy does not appear to be undergoing a major merging event, and has a relatively smooth shape.