The galaxy presents as a centrally concentrated system with a smooth, relatively featureless light distribution. The morphology appears elliptical, displaying a high degree of rotational symmetry. A bright, unresolved core dominates the galaxy's luminosity profile, suggesting a significant concentration of stars and potentially the presence of a supermassive black hole at the galactic center. The color profile appears consistent across the galaxy's extent, with a general yellow-white hue indicating an older stellar population and a low rate of on-going star formation. Faint extensions beyond the core are present; however, the smoothness suggests these extensions are not part of a strong spiral arm or bar feature, more closely resembling an extended halo or envelope. There is no apparent indication of dust lanes or recent merger activity. The galaxy appears isolated, without obvious tidal distortions or nearby companion galaxies.
