The observed galaxy presents a relatively smooth, elliptical morphology. The central region exhibits a concentrated, bright core, indicative of a high stellar density. Proceeding outward from the core, the luminosity gradually diminishes, forming a diffuse halo. A subtle color gradient is discernible, shifting from a slightly yellowish hue in the central region to a bluer tint in the outer regions, potentially suggesting differential stellar populations or dust distribution. Overall, the galaxy appears well-defined and largely undisturbed. There is a subtle irregularity at one edge, suggesting a minor gravitational interaction with a nearby object or possible galactic cannibalism. The elliptical shape appears to be a somewhat elongated, or "in between" circular and cigar shaped. There may be faint indications of tidal features or stellar streams associated with the galaxy, implying past or ongoing interaction with another galaxy or object.
