The galaxy presents as a relatively smooth, disk-shaped structure, viewed at a high inclination. The primary color is reddish, concentrated toward the central bulge, which appears fairly large. Fainter green hues extend along the edges, potentially indicative of areas of active, but low-level, star formation. The overall morphology suggests an older stellar population dominating the light, particularly in the bulge. The disk appears elongated, almost cigar-shaped, indicating a slight asymmetry or distortion. There is no strong evidence of significant tidal features or recent major mergers, suggesting a relatively undisturbed evolutionary history.
