The galaxy presents as an elliptical morphology, exhibiting a smooth, centrally concentrated light profile. The core displays a bright, yellowish hue, suggestive of an older stellar population. Moving outward from the core, the galaxy gradually fades into a bluer halo. There is no discernible spiral arm structure or significant dust lane obscuration. The galaxy is fairly isolated with a high concentration of stars, which could indicate little to no star formation. There are no significant tidal features or signs of recent major merger activity. It is fairly round, with only minor disturbances. 
