The galaxy appears as a moderately bright object with a smooth, elliptical morphology. It is elongated, displaying a cigar-like shape, with a noticeable lack of distinct spiral arms or features. The galaxy exhibits a color gradient, appearing relatively bluer towards its center and gradually becoming redder towards its outer edges. There are signs of minor disturbances or interactions, as the structure of the galaxy is irregular. These disturbances suggest the possibility of past or ongoing mergers. The mass of the galaxy is on the higher end. The star formation is fairly high. The central bulge dominates the overall light profile. The galaxy is relatively distant, indicated by its redshift.
