The galaxy presents as an elliptical morphology, exhibiting a smooth, featureless structure. The central region displays a concentrated, bright core, possibly indicating the presence of a supermassive black hole or a dense concentration of older stars. Moving outward from the core, the light gradually fades, with the outer regions appearing more diffuse. 

Color gradients are noticeable. The central region exhibits a reddish-yellow hue, suggesting an older stellar population dominated by red giant stars. In contrast, the outer regions show a bluer tint, potentially indicative of younger, hotter stars or ongoing star formation, although the lack of distinct spiral arms or HII regions suggests any star formation is relatively quiescent.

The overall shape is elongated, resembling a cigar shape rather than a perfect sphere, suggesting that the galaxy is an elliptical galaxy. There is no visible evidence of recent mergers or tidal disturbances, with no obvious shells or tails.
