The galaxy presents a largely smooth morphology with a concentrated central bulge. The color profile suggests an older stellar population, potentially dominated by redder stars. There is a subtle color gradient, with the central region appearing more yellow and the outer regions exhibiting a slightly redder hue. The galaxy appears relatively undisturbed with no major signs of ongoing merging activity, though the texture of the outer edges suggests a possible minor interaction in the past. The shape of the galaxy appears relatively round with no strong ellipticity. It is likely an elliptical galaxy or a lenticular galaxy with a prominent bulge. Overall, the galaxy has a symmetrical shape with no obvious dust lanes or spiral arms.
