The galaxy presents as a relatively smooth, centrally concentrated object with a generally elliptical morphology. There is a slight elongation to the shape, although it appears mostly rounded. The central region exhibits a brighter, more intense luminosity, suggesting a possible concentration of older stellar populations. Fainter light extends outward from the core, gradually fading into the background sky. There is a very slight asymmetry to the outer edges of the galaxy. No distinct spiral arms or prominent dust lanes are discernible. Overall, the galaxy appears to be relatively undisturbed.
