The galaxy presents as an elongated, elliptical structure. Its overall form appears smooth, lacking distinct spiral arms or irregular features. The central bulge is prominent and exhibits a yellowish hue, indicative of an older stellar population. Moving outward from the core, the color subtly shifts towards a bluer tint in the outer regions. This suggests the presence of younger, hotter stars, indicating ongoing or recent star formation at a modest rate. The galaxy appears relatively undisturbed, with no significant signs of tidal interactions or major mergers. It appears to be a quiescent system. The light profile suggests it could be a moderate-mass galaxy.
