The galaxy presents as a disk-shaped structure, viewed at an oblique angle. A prominent, relatively bright central bulge is observable. The disk itself exhibits a mottled texture, possibly indicating areas of star formation or dust absorption. There are some subtle indications of a spiral structure, but this may be masked by the relatively high inclination of the galaxy's disk. The disk is encircled by an azure-colored ring. The main body of the galaxy is surrounded by a diffuse and faint halo. There is a faint tail-like feature extending from the galaxy, indicative of gravitational interaction. The image shows no obvious signs of a major merger, although subtle disturbances may indicate a minor interaction. Overall, the galaxy appears to be a spiral or lenticular galaxy with some evidence of possible tidal disturbance or interaction.
