The galaxy presents as an elliptical morphology, elongated in shape. It appears relatively smooth in texture, with no significant features such as spiral arms or distinct dust lanes visible. There might be a slight asymmetry, suggesting possible past interactions or mergers. The color profile suggests a mature stellar population, with a reddish hue, indicative of older, cooler stars dominating the galaxy's light output. Star formation is likely subdued, corresponding to the lack of distinct blue regions. The central region is slightly brighter than the outskirts, hinting at a concentrated core.
