The galaxy presents as a smooth, elliptical-like object with a noticeable central bulge. It has a cigar-shaped morphology, appearing elongated rather than circular. There is no evidence of spiral arms or a distinct disk structure. The galaxy exhibits a color gradient, transitioning from a more yellow-white hue in the central region to a slightly bluer periphery. This suggests the presence of older stellar populations concentrated towards the center and younger, possibly star-forming regions in the outer areas, but this is only a slight differentiation. There's no indication of any major mergers or significant tidal disturbances impacting the overall structure.
