The galaxy appears as a centrally concentrated, elliptical-like structure with a generally smooth morphology. The light distribution appears relatively symmetrical, with a gradual decrease in brightness from the core outwards, showing no distinct spiral arm features. The color gradient shifts from yellow in the core towards a more reddish hue in the outer regions, suggestive of an older stellar population dominating the galaxy. There is no evidence of significant tidal disturbances, major mergers or strong interactions with other objects within its immediate vicinity. The galaxy shows a slightly elongated shape.
