The galaxy presents an elongated, cigar-shaped morphology. It exhibits a relatively smooth appearance, suggesting a dominant spheroid component. A faint disk-like structure may be present, viewed edge-on. There's a subtle color gradient across the galaxy, potentially indicating variations in stellar populations or dust distribution along its major axis. No signs of active merging or major tidal disturbances are readily apparent. The overall light distribution is centrally concentrated, though the galaxy appears somewhat diffuse at its outer edges.
