This galaxy presents as a spiral, though the inclination is high, giving it a somewhat lenticular appearance. There's likely ongoing star formation happening within the arms, based on the subtle bluish tint, although it does not appear to be excessively active. A potential minor disturbance or interaction with a smaller, bluer object may be occurring, judging by the proximity and color differences. The galaxy displays some degree of smoothness, yet with the presence of a disk, suggesting it is not a purely elliptical system. Its overall structure doesn't exhibit signs of a major merger event, and the light profile appears to be primarily concentrated in the central region with a gradual fade outward.
