The galaxy presents an elongated, lenticular morphology, appearing as a flattened disk seen edge-on or at a high inclination. The central region exhibits a bright, concentrated bulge, possibly indicating a significant population of older stars. Fainter, diffuse emission extends outward from the bulge along the galactic plane. There appears to be some blue tint present along the outer edges of the disk, perhaps indicative of recent star formation regions. The overall structure suggests a relatively evolved system, though some evidence suggests it may be in a phase of mild star formation. There is no obvious sign of major mergers or significant tidal disturbances.
