The galaxy presents as a generally smooth, elliptical morphology, with no discernible spiral arm structure. The central region exhibits a high degree of luminosity, suggesting a concentrated stellar population and/or active galactic nucleus. There is a slight color gradient, transitioning from a yellow-white core to a redder outer halo, possibly indicating older stellar populations dominating the outer regions. The overall structure appears relatively undisturbed, with no clear signs of major mergers or tidal interactions. The galaxy presents as largely spheroidal and relatively round.
