The galaxy presents as a relatively smooth, centrally concentrated object. The morphology suggests an elliptical galaxy or a spiral galaxy seen face-on with a dominant bulge, possibly of type S0. It exhibits a noticeable color gradient, with the core appearing more yellowish-orange, transitioning to a bluer hue in the outer regions. This suggests a possible decrease in the average age of the stellar population with increasing radius, or a dust lane near the center. No clear spiral arms or prominent features are discernible, with the exception of a subtle asymmetry, hinting at a possible minor interaction or internal disturbance. Overall, the galaxy appears to be a fairly evolved system, likely with a significant stellar mass and a modest star formation rate, concentrated more towards the outskirts.
