The galaxy presents a largely smooth morphology, appearing as a single, centralized object with a high degree of circular symmetry. There are no obvious spiral arms or distinct features indicative of a disk structure. The light distribution is concentrated towards the center, suggesting a prominent galactic nucleus or bulge. The color index indicates a population dominated by older stars, appearing redder than typical spiral galaxies, likely indicating a lower rate of current star formation. There are no signs of ongoing major mergers or significant tidal disturbances; there may be minor interactions occurring, but these do not significantly disrupt the overall smooth appearance.
