The galaxy presents as a disk-shaped structure, viewed at a significant inclination. A central bulge is apparent, exhibiting a yellowish-orange hue. The surrounding disk shows a greenish tint, with hints of spiral arm structure, though the resolution limits detailed tracing. The overall color suggests ongoing star formation, potentially localized within the spiral arms. The morphology appears somewhat disturbed, possibly indicating a minor interaction or recent merger event, or internal disturbances. The galaxy is moderately luminous.
