The galaxy presents an overall elliptical morphology, exhibiting a smooth light distribution with a dominant central bulge. There is a subtle color gradient observed within the galaxy, with the core appearing more yellow indicating an older stellar population, and the outskirts exhibiting a bluer hue, suggestive of ongoing or recent star formation activity. The galaxy has a low star formation rate and high mass. There is no apparent spiral arm structure or significant dust lane features visible. The overall shape is between round and cigar shaped, but closer to being in between the two. There are no major disturbances evident, and the light is relatively symmetric, suggestive of a non-interacting system. There is a possibility of a minor disturbance, but nothing is confirmed. 
