The galaxy presents a somewhat elongated, cigar-shaped morphology. Its light is dominated by a smooth, centrally concentrated component. The color distribution appears relatively uniform across the galaxy, with a noticeable red hue. There is no apparent spiral structure or significant dust lane obscuration visible. While the core is bright, there are no distinct knots of star formation regions or major disturbances detected. The galaxy appears relatively isolated with no obvious signs of tidal interactions or ongoing mergers.
