The galaxy presents as a disk galaxy, observed at a moderate inclination relative to our line of sight. There's a distinct central bulge that appears moderately bright, and a flattened disk component extending outwards. The galaxy exhibits a relatively smooth light distribution, though some subtle features, potentially spiral arm segments, can be discerned within the disk. The disk shows areas of more intense luminosity, suggesting regions of active star formation or higher stellar density. The overall color of the galaxy seems to be trending toward the redder end of the spectrum, indicating a presence of older stellar populations. The outer regions of the galaxy appear less defined, with a gradual decrease in light intensity towards the edges. There are noticeable disturbances, indicating an ongoing or recent merger.
