The galaxy appears to be a relatively luminous object, elongated in shape, potentially a disk galaxy viewed at an angle. It exhibits a smooth, diffuse morphology with a central bulge that seems to dominate the galaxy's overall light profile. There is evidence of possible spiral arm structure, though the arms are not well-defined. The color gradients suggest active star formation regions are present throughout the galaxy, with a higher concentration within the bulge. There are indications of minor disturbances within the galaxy, or possibly an interaction, but these appear minimal and don't drastically affect the overall structure. It is a fairly massive galaxy, with a significant amount of stellar mass.
