The galaxy presents a generally smooth morphology. The central bulge appears dominant and exhibits a yellow-white color, suggesting a population of older stars. A faint disk surrounds the bulge, and a subtle blue tint at the edges suggests the presence of some younger stars. The galaxy exhibits an elliptical shape, leaning toward a more circular appearance. There is no obvious evidence of significant tidal disturbances or ongoing major mergers. The outer regions fade gradually into the background, with no strong indications of active star formation. There is no visible dust. Overall, the galaxy seems to be in a relatively quiescent state.
