This galaxy appears to be a relatively smooth and elongated system. The light is concentrated towards the center, suggesting a substantial bulge component, but no distinct spiral arm structure is visible. The galaxy displays a somewhat cigar-like morphology with an apparent lack of major disturbances. It shows a blue hue, which could indicate ongoing star formation. However, the smoothness suggests it is likely an early-type spiral or lenticular galaxy, likely undergoing minimal star formation, or possibly a dying spiral galaxy.
