The galaxy presents as an elliptical morphology, displaying a smooth light distribution with no discernible spiral arms or bar structure. The light is concentrated towards the center, indicating a prominent galactic bulge. The shape appears somewhat elongated, deviating from a perfectly circular form. Color gradients suggest a possible aging stellar population, with the central bulge exhibiting a yellower, potentially redder, hue compared to the outer regions. There is no obvious evidence of ongoing major mergers or tidal disturbances, the galaxy appearing relatively undisturbed.
