The galaxy presents a compact morphology, appearing nearly circular in shape. The light distribution indicates the presence of a central bulge, with a smooth profile and little evidence of spiral arm structure. There is a slight color gradient, with the central region appearing more red-shifted and the outer regions subtly bluer. There are faint features indicating potential disturbances in the galaxy's structure, suggesting possible past or ongoing minor interactions with other galaxies, but nothing is noticeably asymmetric. The system is observed to have a moderate amount of star formation relative to its mass.
