The galaxy displays a somewhat elliptical morphology, appearing neither perfectly spherical nor significantly elongated. The central region exhibits a high degree of smoothness and a concentrated luminosity, suggesting a significant bulge component. Proceeding outwards from the core, a less distinct and more diffuse structure is observed, hinting at a possible disk-like component or extended halo. There's a subtle irregularity to the overall form. There's a suggestion of disturbed morphology, potentially indicative of a past or ongoing interaction with another galaxy, although not displaying any significant tidal tails. A color gradient is noticeable, with the central region showing a more yellow/orange hue, possibly indicating an older stellar population, while the outer regions appear bluer.
