The galaxy presents as a relatively compact object. Its overall morphology is smooth, exhibiting little in the way of distinct spiral arms or a prominent bar structure. The central region appears brighter and more concentrated, suggesting a possible central bulge or active galactic nucleus. The light distribution gradually fades from the center outwards. There are some mild disturbances to its structure, possibly due to smaller merger events or tidal interactions. The galaxy appears as somewhat in between an elliptical and spiral, showing properties of both.
