The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. Its overall color is notably redder, indicative of an older stellar population and potentially lower levels of ongoing star formation. There is a slight asymmetry to its shape, which could be attributed to minor gravitational interactions or internal dynamics. There is a noticeable lack of prominent spiral arm structures or distinct dust lanes. The luminosity profile appears to be centrally concentrated, gradually fading towards the edges. No signs of a strong bar or ring structure are apparent.
