The galaxy appears as a moderately bright, relatively compact object. It presents a generally smooth morphology, although subtle features hint at a possible disk-like structure. The color profile suggests the presence of both older stellar populations, indicated by reddish hues, and areas of more recent star formation, marked by bluer tinges. The overall shape is somewhat rounded, with a slight deviation from perfect circularity. There is evidence of minor disturbances in the galaxy's structure, potentially indicating past or ongoing interactions. Despite these disturbances, the galaxy does not exhibit signs of a major merger event.
