The galaxy appears to be a spiral galaxy viewed at a moderate inclination. A disk structure is discernable, with a brighter central bulge. There is some indication of spiral arm structure, though the resolution limits detailed observation. The disk appears somewhat asymmetric, potentially due to interactions or internal dynamics. The galaxy exhibits a reddish-orange hue in the central region, suggesting an older stellar population, with a subtle shift towards bluer colors in the outer disk, possibly indicating ongoing star formation in those regions. Dust lanes may be present within the disk but are not clearly resolved. Overall, the galaxy presents a somewhat disturbed morphology, hinting at possible past or current interactions.
