The galaxy presents as a relatively compact and luminous object. It exhibits a morphology that is predominantly smooth and elliptical in appearance, with a high degree of roundness. There's a centrally concentrated bright region, suggesting a possible bulge. The overall color profile appears somewhat redder, potentially indicating an older stellar population. There are subtle, faint extensions surrounding the central region, suggesting a diffuse halo or envelope. The galaxy does not seem to exhibit any obvious signs of ongoing major merging activity, though there might be minor disturbances present.
