The galaxy appears to be an elliptical galaxy, exhibiting a smooth, centrally concentrated light profile. Its shape is elongated, appearing cigar-shaped, indicating a potential E4-E7 classification on the Hubble sequence. The central region displays a brighter, more intense glow, likely corresponding to a dense concentration of older stars. Fainter, bluer hues are discernible in the outer regions, possibly suggesting a small amount of recent star formation activity. The overall structure appears relatively undisturbed, without any signs of major mergers or tidal interactions. The galaxy's moderate redshift places it at a considerable cosmological distance. The estimated mass and star formation rate suggest a galaxy with a relatively high stellar mass and a low to moderate ongoing star formation activity.
