The galaxy presents a generally smooth, elliptical morphology. A central, highly luminous bulge dominates the structure, exhibiting a yellowish hue. The bulge transitions outward to a slightly fainter, more diffuse halo. There's a subtle suggestion of a disk component, though poorly defined with little spiral structure visible. The overall color gradient indicates a higher concentration of older stellar populations within the central bulge, while star formation appears to occur at a modest rate. The lack of significant tidal features suggests that the galaxy is not currently undergoing a major merger, although there is evidence of a minor disturbance. The galaxy appears approximately round in shape.
