The galaxy presents a generally smooth, elliptical morphology, exhibiting a concentrated central bulge that radiates brightly in yellowish hues. This central region gradually fades into a less distinct and more diffuse outer halo. The overall shape is somewhere between round and elongated, with the image suggesting a system that is neither perfectly spherical nor heavily distorted into a cigar shape. There is little evidence of strong spiral arm structure or active merging events with other galaxies; however, a slight asymmetry in the outer regions hints at a possible minor disturbance or interaction in the galaxy's recent past. The galaxy displays a color gradient, with the core appearing more yellow suggesting an older stellar population, while the outer regions show a hint of bluer tones, indicating the presence of younger stars, albeit in a seemingly suppressed star formation environment.
