The galaxy presents as a relatively smooth, elliptical structure. The central region exhibits a bright, concentrated core, suggesting a higher density of stellar populations. The overall color appears bluish-white, which may indicate the presence of younger, hotter stars. There is little evidence of distinct spiral arms or prominent dust lanes, supporting the classification as elliptical. The galaxy’s morphology is generally elongated, with a slight cigar shape. There are no obvious signs of major mergers or significant tidal disturbances, although minor disturbances may be present.