The galaxy appears to be a spiral type, exhibiting a notable central bulge and a disk. The bulge is a strong orange color and is relatively large compared to the disk, indicating an older stellar population and possibly an active galactic nucleus. One side of the galaxy disk appears to be more extended than the other, suggesting a possible interaction or tidal disturbance, this side is bluer in color and a very light hue. The disk itself shows a hint of spiral arm structure, although it is somewhat faint and diffuse. The color gradient suggests star formation is suppressed. Overall, it is a moderately luminous object with signs of past or ongoing interaction shaping its morphology.