The object appears to be a galaxy with a prolate, or cigar-like, morphology. A concentrated central bulge exhibits a yellowish hue, potentially indicating an older stellar population. Extending outward from the bulge, there is a fainter, bluish disk. The disk may contain regions of more recent star formation. There is evidence of possible minor disturbances in the structure, which could be due to interactions with other galaxies. Overall, the galaxy presents a relatively smooth profile but is neither perfectly elliptical nor a clearly defined spiral structure. The estimated size of the galaxy is roughly 10 kpc in radius. The estimated redshift places the galaxy at a significant cosmological distance. The mass and low star formation rate may indicate that the galaxy is a late-type spiral galaxy, currently evolving to a more spheroidal morphology.
