The galaxy presents as a relatively smooth, elongated object, likely an elliptical galaxy or a lenticular galaxy viewed at an angle. There is a pronounced central bulge, appearing more concentrated and yellowish in color, suggestive of an older stellar population. The galaxy lacks well-defined spiral arms or significant dust lanes. The outer regions display a bluer hue compared to the core, potentially indicating the presence of some younger stars but to a much lesser extent. Overall, the galaxy's morphology appears regular with no noticeable major disturbances or signs of ongoing mergers.
