The galaxy presents as a flattened, elliptical shape with a clear major axis. It exhibits a smooth morphology, lacking distinct spiral arm structures or prominent dust lanes. The core region appears brighter and more concentrated, suggesting a higher density of stars. A subtle color gradient is observable, with the central regions displaying a yellowish hue potentially indicative of an older stellar population, while the outer regions show hints of bluer tones suggesting the presence of younger, hotter stars, though this is more subdued. The overall light distribution is diffuse, fading gradually from the center outwards. Based on its shape, smooth texture, and color profile, the galaxy is likely an early-type galaxy, perhaps an elliptical or lenticular type. There is no obvious indication of ongoing major mergers or significant tidal disturbances.
