The galaxy exhibits a relatively smooth, elliptical morphology. There is minimal evidence of spiral arm structure or significant dust lanes within the central region, suggesting a more evolved stellar population. The color profile shows a subtle redder hue towards the core, implying an increased concentration of older stars. The overall symmetrical shape indicates it is likely not undergoing a major merging event, despite some minor asymmetries in the outer isophotes. There is very little discernible new star formation within the galaxy.