The galaxy presents as a yellowish-orange elliptical. Its morphology appears relatively smooth, with no distinct spiral arm structures or prominent dust lanes visible in this image. There is a slight elongation, suggesting a departure from perfect circularity, tending more towards an in-between shape. No obvious signs of ongoing major mergers or tidal disturbances are observed, although minor disturbances cannot be entirely ruled out. Given its color and smoothness, the galaxy appears to be relatively quiescent, indicating a potentially older stellar population with suppressed star formation. The absolute magnitudes are within reasonable values, with a strong inclination of the galaxy to show its redder characteristics. The overall light profile is consistent with a galaxy dominated by evolved stars.
