The galaxy presents as a relatively smooth, elliptical structure. It exhibits a central bulge that appears bright and concentrated, transitioning gradually to a less luminous, more diffuse outer region. The color gradient suggests a population of older stars dominating the central bulge, with a subtle bluish hue in the outer disk, possibly indicating some ongoing star formation. The overall morphology is generally undisturbed, with no obvious signs of tidal interactions or major mergers. There's a slight elongation, suggesting it's not perfectly spherical. No spiral arm structures are apparent.
