The galaxy presents as a luminous, elliptical object. Its overall shape is smooth and somewhat elongated, displaying an intermediate axial ratio; it is neither perfectly circular nor highly flattened. The central region exhibits a high concentration of light, suggesting a prominent nucleus or bulge. The light profile gradually fades from the center outwards, lacking any distinct spiral arm structures or prominent dust lanes. The color appears largely uniform throughout the galaxy, with a general yellowish/orange hue. This color suggests a stellar population dominated by older, redder stars, with limited ongoing star formation. There is minimal evidence of any major mergers or tidal disturbances, though subtle asymmetries in the outer regions might indicate minor interactions in the past.
