The galaxy presents a largely smooth morphology, suggestive of an elliptical type. It exhibits a centrally concentrated, bright core that gradually diffuses outwards into a halo-like structure. The overall shape is relatively circular, with minimal deviation from a spheroidal form. There's a subtle color gradient visible, transitioning from a yellower hue near the center to a redder tinge in the outer regions. This may indicate a variation in stellar populations, with older, redder stars dominating the outskirts. No prominent spiral arms, bars, or distinct features of active star formation are discernible. There are no signs of major mergers or significant tidal disturbances, though some slight irregularities in the outer halo might suggest minor interactions in its past. The lack of substantial disk-like features and the smooth, centrally concentrated light distribution strongly point toward a galaxy with a relaxed, evolved stellar population.
