The galaxy appears to be a relatively smooth, centrally concentrated system. It exhibits an elliptical morphology, with a high degree of central concentration and a noticeable lack of distinct spiral arms or bar structures. The light profile suggests a relatively old stellar population, with a smooth gradient from the core outwards. There is a suggestion of a disk like structure, though it is not prominent. The galaxy does not appear to be undergoing any major merging events, though minor disturbances cannot be ruled out. The color profile indicates a moderate amount of on-going star formation within the galaxy, contributing to its overall luminosity. The effective radius appears to be relatively compact, suggesting a moderate overall size for this galaxy.
