The galaxy presents as a relatively small, disk-shaped object with a bright, concentrated central bulge. The overall color appears predominantly greenish-white, with an inner region of intense brightness suggesting a significant stellar population or active galactic nucleus. Faint extensions are visible surrounding the central region, possibly indicating the presence of a galactic halo or extended disk. Some subtle color variations exist across the galactic disk, with hints of redder hues on the edges, suggesting differential stellar populations or dust obscuration. The overall smoothness of the disk is only moderate, perhaps suggesting some level of disturbance or interaction, however no dominant features or spiral arms can be observed. The galaxy appears to be non-interacting with any apparent merger activity, but appears to be slightly irregular.
