The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge of high luminosity, surrounded by a more diffuse halo. There is a subtle hint of a disk-like structure around the core, but no distinct spiral arms are discernible. There's a slight asymmetry to the overall shape; disturbances may be present in the outer regions of the galaxy. The color gradients suggest a potentially evolved stellar population, with redder hues at the edge of the disk. There seems to be some recent star formation occurring towards the central region, suggested by the bluer color in the core. Overall, this galaxy appears to be a relatively massive system, with evidence of ongoing, albeit possibly declining, star formation.
