The galaxy appears to be a relatively smooth, elliptical or lenticular system. Its morphology suggests a high degree of sphericity; the light distribution is concentrated towards the center, displaying a bright, diffuse core that diminishes gradually outwards. There is a subtle color gradient, with the core exhibiting a slightly yellower hue compared to the outer regions, potentially indicating a population of older stars in the central bulge. There is no evidence of prominent spiral arms, strong dust lanes, or active star-forming regions. The galaxy shows no strong signs of tidal disturbances or ongoing merger activity. It exhibits a generally undisturbed, relaxed structure.
