The galaxy presents an elliptical morphology, exhibiting a smooth light distribution without discernible spiral arms or bar structures. The color gradient indicates a relatively older stellar population dominating the central region, evidenced by the yellowish-orange hue which likely represents the integrated light from evolved stars. This core gradually transitions to a greenish-blue halo or outer disk, possibly indicating the presence of a younger stellar population and/or ongoing, though subdued, star formation activity. The galaxy appears relatively isolated, showing no obvious signs of tidal interactions or major mergers, although minor disturbances cannot be entirely ruled out given the slight asymmetry in the outer regions. Its overall structure suggests an evolved system that is approaching quiescence in terms of star formation.
