The galaxy presents as a largely featureless, elliptical object. It exhibits a smooth, centralized light distribution with a high degree of radial symmetry. The core region appears intensely luminous, with a color gradient trending towards redder hues, suggesting an older stellar population. There is no discernible spiral structure or evidence of active star formation within the visible spectrum. Faint diffuse light extends outwards from the central region, gradually decreasing in intensity with radial distance. The galaxy does not exhibit any obvious signs of tidal disruption or interaction with other galaxies.
