The galaxy exhibits a lenticular morphology, appearing as a flattened disk seen edge-on. There is a smooth, diffuse bulge component that dominates the central region, with a distinct disk extending along the major axis. The disk appears relatively thin and featureless. The color profile suggests a higher concentration of older stellar populations. Some faint and smaller blue clumps appear throughout the disk which may be areas of recent star formation. There are no apparent signs of spiral arms or prominent dust lanes, further suggesting a more evolved, quiescent system. The overall appearance is consistent with a galaxy undergoing a transition from a spiral to an elliptical morphology, or a dwarf galaxy with a somewhat irregular structure.
