The galaxy presents as a slightly elongated, disk-shaped structure with a dominant central bulge. The overall color appears bluish, suggesting the presence of younger, hotter stars. The central bulge appears somewhat more concentrated and displays a slightly whiter hue, potentially indicating a higher density of older stars, or possibly a region of active galactic nuclei. There is a hint of spiral structure, but it's not clearly defined. The disk appears relatively smooth with limited visible dust lanes. A possible minor disturbance is indicated by the slight asymmetry in the outer regions of the disk. There may be a neighboring, smaller galaxy close by.
