The galaxy presents as a relatively compact, elliptical system. Its morphology appears predominantly smooth, with a high degree of radial symmetry. The light distribution suggests a centrally concentrated bulge component dominating the overall structure. There is a lack of discernable spiral arms or prominent disk features. The color profile indicates a redder population, characteristic of older stellar populations. Overall, the galaxy does not exhibit signs of ongoing major mergers or significant tidal disturbances.
