The galaxy presents a somewhat elliptical morphology. The central region is bright, exhibiting a high concentration of light, potentially indicating a substantial galactic nucleus. The light profile appears to gradually diminish outwards from the center, suggesting a fairly smooth distribution of stars or ionized gas. The galaxy appears to have a slight disk, which is close to edge-on. There are no obvious spiral arm structures, dust lanes, or prominent star-forming regions visible. There does not seem to be any major signs of galaxy interaction, although there might be a minor disturbance to the shape. The overall color is bluish in the center, transitioning to redder hues in the outer regions, which may suggest older stellar populations in the outskirts. The elliptical shape appears to be closer to a cigar shape.
