This galaxy exhibits an elliptical morphology, presenting a generally smooth appearance with a centrally concentrated bulge. The light distribution suggests that the galaxy has a predominantly older stellar population. The overall color profile indicates a moderate amount of ongoing star formation, which is not very active. The object appears slightly elongated, departing from a perfectly spherical shape. There is no evidence of a major merger event. However, the morphology indicates that the galaxy may have minor interactions with other galaxies. There is a possibility of a slight disturbance in the disk.
