The galaxy presents a generally smooth, elliptical morphology. It appears relatively undisturbed, lacking prominent spiral arms or tidal features indicative of recent major mergers. The galaxy exhibits a somewhat round shape, though a slight elongation is discernible. Color gradients suggest a concentration of older stellar populations towards the core, with a yellowish hue predominating. The overall structure is centrally concentrated, with luminosity gradually decreasing towards the outer regions. Faint, diffuse features are observed in the outskirts, potentially indicative of a faint stellar halo or past minor interactions. No strong dust lanes or regions of active star formation are immediately apparent in this image.
