The galaxy presents as a relatively smooth, elliptical morphology. The color is predominantly yellow-orange, indicating an older stellar population, with reduced recent star formation. There is no obvious dust lane or spiral arm structure. The galaxy exhibits a centrally concentrated bulge, with a gradual decrease in luminosity towards its outer regions. The shape is generally round, without significant elongation or distortion suggestive of recent mergers or interactions. The object appears as a single, distinct entity, with no clear indication of tidal features or companion galaxies that would suggest recent merger activity, though low level disturbances are not out of the question.
