The galaxy presents as a centrally concentrated object with a generally elliptical morphology. A smooth, diffuse component dominates the light profile. The central region exhibits a yellowish-orange hue, suggesting an older stellar population. Fainter, bluer extensions are observed beyond the central bulge, hinting at the presence of a disk-like structure. However, distinct spiral arms or bar features are not readily apparent. There might be some minor disturbance in the galaxy shape, with possibly some merging activity. The overall impression is that this is a massive, relatively evolved system with modest ongoing star formation.
