The galaxy presents a generally smooth, elliptical morphology with a high degree of central concentration. The light distribution appears radially symmetric, lacking any discernible spiral arms or bar structures. A prominent, bright core dominates the galaxy's luminosity profile. The galaxy exhibits a color gradient, transitioning from a yellowish-white central region to a slightly bluer halo. This suggests a population of older, redder stars concentrated in the core, with younger, bluer stars residing in the outer regions. The galaxy lacks any obvious signs of ongoing major mergers or significant tidal disturbances, although a subtle asymmetry hints at a potential minor interaction in its past. Overall, this galaxy appears to be a relatively undisturbed, evolved system.
