The galaxy appears to be relatively small, with an apparent magnitude suggesting it is quite faint. The overall morphology is somewhat difficult to discern due to limited resolution, but it seems to exhibit a disk-like structure, possibly an irregular or disturbed morphology. There is a hint of a central bulge, with a smoother appearance compared to the outer regions. The color distribution suggests the presence of both older stellar populations, indicated by reddish hues, and possibly some younger, bluer stars scattered within the disk. The disk appears asymmetrical, with some possible tidal features or disturbances suggesting gravitational interaction with another galaxy or recent merger event. There are some regions of increased brightness scattered throughout the galaxy that could be star forming regions or unresolved stellar clusters. The galaxy does not appear to be a perfect elliptical nor a spiral but somewhat in-between, potentially an intermediate galaxy type.
