The galaxy presents a lenticular morphology, appearing as a flattened disk with a bright, concentrated central bulge. The disk component shows a faint blue tinge, suggesting some level of ongoing star formation, though not at a high rate. The central bulge exhibits a yellowish-orange hue, indicative of an older stellar population. The overall structure appears relatively undisturbed, showing no significant signs of recent major mergers or tidal interactions. There are some minor disturbances visible in the disk, but they do not seem to greatly affect the overall morphology. The galaxy is relatively compact, implying it is not a very large galaxy. 
