The galaxy presents a generally smooth, elliptical appearance. There is a concentrated central bulge with a diffuse surrounding halo. Color gradients suggest a slightly redder core, potentially indicating older stellar populations concentrated towards the center. Fainter, bluer regions are observed in the outer edges of the galaxy, implying some level of ongoing or recent star formation. The overall structure appears largely undisturbed, with no obvious signs of a major merger event or significant tidal interactions. The galaxy is somewhat elongated, but generally rounded in shape.
