The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology appears to be largely elliptical, showing a high degree of radial symmetry with a slight deviation towards a less-rounded shape. There are no distinct spiral arms or a prominent disk visible. The galaxy exhibits a generally even color distribution, with a hint of a redder hue towards its core, likely indicating an older stellar population. The overall light profile suggests a lack of significant recent star formation, aligning with the color gradient observed. There is no obvious evidence of ongoing mergers or tidal disturbances in the immediate vicinity of the galaxy.
