The galaxy appears to be a relatively smooth, elliptical structure. The central region exhibits a high concentration of light, suggesting a prominent galactic nucleus. There is little evidence of spiral arms or significant disk structure in the image. The object is somewhat round in shape, rather than elongated or cigar shaped. Overall, it does not appear to be undergoing any major mergers or exhibiting strong tidal disturbances, although some minor disturbances cannot be ruled out at this resolution. The galaxy exhibits a moderately high redshift, suggesting that it is a relatively distant object.
