The galaxy presents as a luminous, elliptical structure, exhibiting a relatively smooth morphology with no discernible spiral arm features. The central bulge appears bright and concentrated, suggesting a high density of older stellar populations. A slightly less luminous region sits below the bulge, perhaps indicating recent interactions. The color profile is dominated by warmer tones, implying a population of older stars and a lower rate of active star formation. There is no evidence of a prominent dust lane or significant disturbances in the overall structure, suggesting a relatively relaxed dynamical state.