The galaxy presents as a relatively smooth, elliptical-shaped object with a noticeable bulge. The central region exhibits a yellowish-orange hue, indicative of an older stellar population. Progressing outwards from the center, there is a gradual shift towards a bluer tint, which may suggest the presence of younger stars within the galaxy's disk. The disk appears to be tilted relative to our line of sight, giving the galaxy its elongated appearance. There are no strong indications of spiral arm structures or significant dust lanes visible in this image. Overall, the galaxy appears to be relatively isolated, with no obvious signs of major interactions or mergers. Based on its morphology, the galaxy is likely a relatively massive system, potentially with ongoing, but moderate, star formation activity.
