The galaxy presents a generally smooth, elliptical morphology. The central bulge is prominent, exhibiting a bright, concentrated luminosity. The surrounding disk, though visible, appears less defined, indicating a relatively low fraction of organized structures such as spiral arms or distinct dust lanes. The overall shape is closer to being cigar-shaped rather than fully rounded. There may be some minor asymmetry or a subtle indication of past interaction, but no prominent signs of a major merging event are observed. In terms of color distribution, the central regions appear somewhat yellower or whiter, possibly indicating an older stellar population, with the outer regions exhibiting a bluer hue, which may indicate recent star formation.
