The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a predominantly elliptical morphology, with a slight deviation from perfect circularity. The central region displays a high surface brightness, indicating a significant concentration of stars or an active galactic nucleus. The galaxy's color is generally yellowish-white, suggesting a population of older stars with lower star formation activity. There are no discernible spiral arms or prominent dust lanes. Faint, diffuse light extends outwards from the central region, fading gradually into the background. Overall, the galaxy appears to be a quiescent, evolved system with little ongoing star formation. There are some indications of minor disturbances in the galaxy's morphology, but they are not significant enough to classify this as a major merging event.