The galaxy presents as a somewhat elongated, disk-like structure seen at a moderate inclination, but not quite edge-on. The central region exhibits a brighter, more concentrated glow, suggestive of a central bulge. The color appears to transition from a yellow-orange core outwards to fainter, bluer hues in the outer disk. The disk appears somewhat disturbed or warped. There may be signs of a minor interaction or tidal disturbance, which could explain the irregular shape. There isn't a clear indication of strong spiral arm structure, suggesting this might be an older disk galaxy or one that has experienced recent interactions that disrupted its spiral pattern. Overall, the galaxy exhibits characteristics consistent with a moderately massive system undergoing or having recently undergone some form of interaction or disturbance that influences its morphology and star formation.
