The galaxy appears to be an elliptical type, exhibiting a smooth, centrally concentrated light profile. It has an overall elongated shape, approximating a cigar-like form. The core region appears brighter and more yellow in color, potentially indicating an older stellar population. Moving outward from the core, the galaxy shows a gradual decrease in luminosity. There is a possible subtle blue-ish tint toward the outer edges, which may indicate the presence of some younger stars. There are no apparent spiral arms, dust lanes, or other distinct features that would characterize a spiral or irregular galaxy. There are no signs of major tidal disturbances or ongoing mergers, although some minor disturbances cannot be ruled out. The observed redshift suggests that the galaxy is at a considerable distance.
