The galaxy appears as a relatively smooth, elliptical structure. Its core presents a bright, concentrated luminosity, suggestive of a high stellar density. The radial color gradient indicates a shift from a yellowish core to a redder outer halo, possibly signifying an older stellar population in the outer regions compared to a more actively forming stellar population at the core. There are no apparent spiral arms or significant dust lanes visible, supporting a classification toward the elliptical end of the Hubble sequence. The morphology is largely undisturbed, exhibiting no signs of ongoing major mergers or significant tidal disruptions. The observed light distribution suggests that it is a galaxy with a substantial mass and limited current star formation activity, implying an evolved system with a stable, quiescent state.
