The galaxy presents a largely smooth, elliptical morphology. A concentrated central bulge is evident, exhibiting a bright yellowish-orange color, likely indicative of an older stellar population. Fainter, extended light surrounds the core, fading gradually into the background. This suggests a more diffuse stellar distribution in the outer regions. There is little evidence of distinct spiral arm structures or significant dust lanes. The overall shape appears relatively rounded. Possible minor asymmetry in the light distribution may suggest a past interaction, but no major tidal features or obvious signs of an ongoing merger are visible. The galaxy's color profile, from the core outwards, suggests a gradient with the bluest regions being the furthest out from the core.