The galaxy presents a flattened, disk-like structure with a significant bulge. The central region exhibits a concentrated luminosity gradient, transitioning to a fainter, extended halo. The overall color profile suggests a relatively evolved stellar population. There may be dust, judging from the slightly redder color. The galaxy appears relatively undisturbed, showing no signs of major merger events. There also appears to be some evidence of star formation, possibly in the inner ring, judged from the blue color there. The orientation is close to edge on.
