The galaxy appears as a relatively compact, elliptical structure. It presents a smooth, fairly uniform light distribution across its body, suggesting a dominance of older stellar populations. The overall color is slightly reddish, consistent with a population of evolved stars and potentially a low level of ongoing star formation. There are some hints of structural irregularity, possibly the result of past merger events. A weak tidal feature may be present in the upper part of the galaxy. There is evidence of some mild disturbance, possibly due to gravitational interactions or internal processes, which contribute to the overall morphology. The galaxy is of considerable size, with an estimated effective radius of approximately 7 kpc, indicating a substantial stellar mass.
