The galaxy appears to be a relatively bright, elongated object, likely a spiral or lenticular galaxy viewed at an oblique angle. Its color suggests ongoing star formation, particularly in its central region, though the overall color profile indicates a mix of stellar populations. The galaxy exhibits a dominant, smooth component with a bright nucleus, suggesting an older stellar population concentrated in the bulge. There are hints of disk-like structure surrounding the bulge, though it is not clearly defined. The shape indicates that it is likely a somewhat flattened, rotating system. The color index would imply that it has gone through a stage of star formation and has undergone a period of little star formation with little dust content. There is a faint tidal feature or merging galaxy that may be indicative of some disturbance.
