This galaxy exhibits a relatively smooth morphology, with a noticeable elongated, cigar-like shape. The central region presents a bright, concentrated luminosity that appears yellowish in color, potentially indicating a population of older stars. Progressing outward from the core, the galaxy fades gradually into a bluish hue, which could suggest the presence of a younger, star-forming stellar population within the galactic disk. The smooth appearance suggests that the galaxy is relatively undisturbed, showing no major signs of recent mergers or tidal interactions. There are some subtle irregularities at the edges of the galaxy, suggesting that it has experienced some minor interaction at some point in its history.