The galaxy presents as a cigar-shaped, elliptical morphology. It exhibits a smooth, featureless appearance, lacking any readily discernible spiral arms or distinct disk structure. There are no obvious signs of recent or ongoing major mergers or significant tidal disturbances. The galaxy displays a color gradient, appearing relatively bluer at its outer edges and transitioning towards a redder hue in its central region, possibly indicating a higher concentration of older stellar populations towards the core. Given its observed properties, this galaxy is likely an elliptical galaxy, with an estimated stellar mass on the order of 10^10 solar masses. Its estimated star formation rate suggests it is actively forming stars at a modest rate, with a specific star formation rate indicating a relatively low level of ongoing star formation relative to its total stellar mass.
