The galaxy presents as a somewhat elongated, elliptical shape with a smooth, diffuse light distribution. Its color profile indicates a generally older stellar population, with a slightly brighter, bluer central region suggesting recent star formation. The galaxy appears undisturbed, showing no signs of major mergers or tidal interactions. There are hints of spiral arms or disk-like structures, but they are faint. Overall, the galaxy seems to be a mid-mass system with a moderate rate of star formation.