The galaxy exhibits a smooth, elongated morphology, appearing cigar-shaped. Its central region is characterized by a higher concentration of light, suggesting a prominent bulge. The color profile indicates a relatively evolved stellar population, with a general yellowish-white hue throughout the galaxy, particularly in the central bulge. There's a subtle blue tint on the edges, possibly indicating a small amount of more recent star formation, but the bulk of the light appears to be coming from older stars. No distinct spiral arms or significant dust lanes are visible, and the galaxy lacks any obvious signs of major tidal disturbances or ongoing mergers.
