The galaxy presents a relatively smooth, elliptical morphology. A bright, concentrated central bulge dominates the overall structure, exhibiting a yellowish hue, indicative of an older stellar population. The surrounding halo appears less concentrated and displays a bluer color, suggesting the presence of younger stars or a more diffuse distribution of stellar populations. There is a subtle elongation to the galaxy's shape, though it is primarily round. No distinct spiral arm structure or prominent dust lanes are visible. Faint hints of a disturbance in its outer regions suggest a possible past interaction or minor merger event.