The galaxy presents as an elliptical morphology. It exhibits a relatively smooth, centralized concentration of light with a radial gradient decreasing outwards from the center. There is minimal visual evidence of spiral arm structure or significant dust lanes. The galaxy appears moderately round. There is no strong morphological evidence of major ongoing mergers. A slight asymmetry may hint at a past interaction or minor disturbance. The color profile suggests an older stellar population, with the galaxy appearing more red than blue. The estimated effective radius of the galaxy is approximately 7.6 kpc, indicating a substantial, but not exceptionally large, physical size.
