This galaxy presents as an elliptical morphology. The light distribution appears smooth and concentrated towards the center, suggesting an older stellar population. The galaxy appears nearly round, with a slight elongation. There is no apparent evidence of spiral arms or significant dust lanes. The light profile exhibits a centrally concentrated bulge. The color is generally reddish, indicative of a population of evolved stars. There is no visually apparent ongoing major merging activity, though minor disturbances cannot be ruled out.
