The galaxy presents as a singular, relatively smooth object with a high degree of central concentration. It appears roughly circular in shape, exhibiting a mild degree of elongation. There is a color gradient apparent, with the central region displaying a yellowish-white hue, transitioning to a slightly reddish tint in the outer regions. There is little visible evidence of spiral arm structure or significant dust lanes, suggesting a morphology leaning towards an elliptical type. The overall faintness and color characteristics suggest a galaxy with a comparatively older stellar population, and a low rate of star formation, though some star formation is likely occurring. Some minor tidal disturbance is possible, given slight asymmetries in its shape.
