The galaxy presents as a somewhat smooth, centrally concentrated object. It exhibits a generally elliptical morphology, appearing mostly round but with a slight elongation. The galaxy’s color profile suggests a primarily older stellar population, indicated by the yellowish-red hue dominating the central region. However, there are subtle hints of bluer regions, suggesting some ongoing, albeit limited, star formation. There is morphological evidence of a possible interaction or merger event in the recent past. A few bright spots may be from active galactic nuclei or unusually bright star forming areas. Overall, the galaxy shows evidence of being a significant mass object.
