The galaxy presents a smooth, elliptical morphology, characterized by a concentrated central bulge. The light distribution appears relatively uniform, lacking distinct spiral arms or other prominent features. The color profile suggests a population of older stars, indicated by a yellow-red hue. There is no apparent dust lane obscuring the central region, and the galaxy appears to be relatively undisturbed, with no evidence of significant tidal interactions or mergers. The overall shape is nearly circular, with a slight deviation toward an ellipsoidal form. Given the morphology, we can infer a relatively low star formation rate.
