The object appears to be a galaxy, likely at intermediate redshift. It exhibits an elongated, cigar-shaped morphology. The central region is brighter and appears yellowish-orange, possibly indicating an older stellar population and/or dust obscuration. There is a hint of bluer, fainter emission extending away from the central region on either side, suggesting the presence of younger stars or star-forming regions in a possible disk or spiral arm structure. The galaxy exhibits a generally smooth appearance, with a subtle indication of minor disturbance in its overall structure, although there are no clear signs of a major merger event currently taking place.
