The galaxy presents as a relatively compact, elliptical morphology. It exhibits a centrally concentrated brightness profile, with luminosity decreasing radially outward. The overall color is suggestive of an older stellar population, with a notable absence of strong blue emission indicative of recent or ongoing star formation. There is a subtle color gradient, with the central region appearing slightly redder than the outer halo. The isophotes appear to be largely smooth and regular, with no obvious signs of strong tidal features or major morphological disturbances. Faint, extended halo is barely noticeable and fairly circular, gradually blending into the background sky.
