The galaxy presents as a lenticular or early-type spiral galaxy, appearing elongated with a notable bulge. The central bulge appears to dominate the overall light output, exhibiting a smooth, concentrated distribution with a yellowish hue. Fainter, bluer regions are observed primarily along the edges of the galaxy, suggesting possible areas of more recent star formation, but these are not very pronounced. There is no obvious dust lane and the overall structure is relatively undisturbed, indicating a lack of recent major merger events. It has a considerable size. There may be an indication of a disk component but it is very faint.
