The galaxy presents a generally smooth morphology, with minimal discernible features such as spiral arms or a prominent central bulge. It exhibits a nearly circular profile. The light distribution suggests a centrally concentrated structure, with a gradual decrease in luminosity outward from the core. The galaxy exhibits a color gradient, transitioning from a bluer hue in the outer regions to a more yellowish-red towards the center, suggestive of potential variations in stellar populations or dust content. There appears to be no significant indication of tidal disturbances, mergers, or interactions with neighboring galaxies.
