The galaxy presents a somewhat smooth, elliptical morphology, appearing more elongated than perfectly spherical. The light distribution suggests a centrally concentrated bulge, which transitions into a fainter, more diffuse halo. There is a subtle hint of a disc-like structure, but it is not clearly defined and possibly contains some features or arms. The color profile suggests a population of older stars, contributing to the redder hue, particularly in the central region. There may be a presence of some ongoing, though relatively low, star formation activity occurring in the galaxy. Based on its characteristics, it is unlikely that the galaxy is undergoing a major merging event, although minor disturbances cannot be ruled out.
