The galaxy presents as an elliptical type, with a smooth, diffuse morphology and no apparent spiral arm structure. The central bulge is prominent and exhibits a concentrated, bright yellow-orange hue, suggesting an older stellar population. Moving outward from the center, the luminosity gradually decreases. The outer regions display a slightly bluer tint compared to the core, potentially indicating the presence of a younger stellar population. The overall shape deviates moderately from perfect circularity, appearing somewhat elongated. There is no clear evidence of significant tidal distortions or ongoing major merger activity, although minor disturbances cannot be ruled out.
