The galaxy presents a generally smooth and concentrated morphology. It exhibits a centrally bright and prominent bulge that dominates its overall luminosity. The bulge region appears roughly elliptical in shape, transitioning smoothly into a fainter, more diffuse halo or disk component surrounding it. There is a slight elongation to the shape of the galaxy, moving towards a cigar shape, although it is mostly in between round and elongated. There is no evidence of strong spiral arm structure or significant dust lane obscuration visible in this image. There are no major merging components.
