This galaxy exhibits a morphology that leans towards a spiral type, although with noticeable peculiarities. It has a central bulge region that appears yellowish, suggesting an older stellar population. The disk component is prominent, displaying hints of spiral arm structure, although the arms are not well-defined and appear somewhat flocculent.

There's a suggestion of tidal disturbances or interactions, indicated by asymmetry in the disk and possible faint extensions or plumes of stellar material extending from the main body. The overall color of the disk is bluer compared to the bulge, which could indicate the presence of younger, hotter stars and ongoing star formation.

Given the apparent size and luminosity, this galaxy is likely a relatively massive system with a significant rate of star formation. The features observed suggest it may be undergoing or has undergone a minor merger event that is influencing its current structure and star formation activity. Further spectroscopic studies are warranted to confirm its redshift, stellar population properties, and the nature of any interactions.
