The galaxy presents as a relatively smooth, elliptical structure. The central region exhibits a concentrated, bright core, suggesting a higher density of stars and possibly an active galactic nucleus. There is a subtle color gradient, with the core appearing more yellow, possibly indicating an older stellar population, and the surrounding region having a slightly bluer tint, hinting at ongoing star formation. The overall morphology lacks any distinct spiral arms or bar structures, further supporting its classification as an elliptical galaxy. The faint, diffuse outer regions gradually blend into the background, showing little evidence of tidal interactions or recent merger events. A slight asymmetry could indicate a minor interaction, but generally the galaxy appears relaxed and undisturbed.
