The galaxy presents a largely smooth, elliptical morphology, although there are subtle suggestions of a disk-like structure within the broader halo. Its light distribution is concentrated toward the center, which appears bright and yellowish, possibly indicating an older stellar population. Moving outward, the color transitions to a bluer hue, hinting at some ongoing, though perhaps not vigorous, star formation in the outer regions. The galaxy shows minimal signs of major disturbances, though a slight asymmetry might suggest a minor interaction or tidal feature. Overall, this galaxy appears to be a relatively evolved system, potentially in a transition phase between a more actively star-forming spiral and a quiescent elliptical.
