The galaxy presents a generally elliptical morphology, exhibiting a smooth, centrally concentrated light distribution. The central region displays a pronounced orange-red hue, suggesting a population of older, redder stars and/or significant dust obscuration. Moving outwards from the core, the color shifts towards a slightly bluer, greenish tint, potentially indicating the presence of younger stellar populations or a decrease in dust content. Faint, diffuse outer regions are visible, extending further along the major axis of the ellipse. No obvious spiral arm structures or distinct features are readily apparent, suggesting a relatively evolved or quiescent system. Minor irregularities in the outer halo may imply past interaction or accretion events. The overall appearance points towards a galaxy with a dominant bulge component.