This galaxy presents as a disk galaxy, viewed nearly edge-on. It exhibits a prominent central bulge, characterized by a high surface brightness and a yellowish-white color, indicative of an older stellar population. The disk component appears relatively thin and elongated, with a noticeable blue tint. The bluer color suggests the presence of younger, hotter stars and ongoing star formation within the disk. There is some indication of dust lanes or patchy structures within the disk, although the resolution is not high enough to resolve individual star-forming regions. Overall, the galaxy displays a relatively smooth morphology, with no strong evidence of major mergers or significant tidal disturbances.
