This galaxy exhibits a generally smooth morphology, appearing largely spheroidal in shape. The light distribution is concentrated towards the center, with a gradual decrease in brightness extending outward. The central region shows a yellow-white hue, suggesting a population of older stars. There is minimal evidence of spiral arm structure or a prominent disk component. Faint irregularities in the outer regions may suggest minor tidal disturbances or interactions with smaller companions, although a major merger event appears unlikely. The galaxy does not display any significant dust lanes or active star-forming regions. The roundness of the central bulge implies a minimal degree of oblateness.
