The galaxy presents as an elongated, disk-like structure, oriented nearly edge-on with respect to our line of sight. A central bulge is apparent, exhibiting a brighter, more concentrated luminosity profile compared to the outer regions of the disk. The bulge appears somewhat yellowish in color, suggesting an older stellar population. The disk itself shows subtle color gradients, with bluer hues potentially indicating regions of more recent star formation. While no prominent spiral arms are immediately discernible, subtle irregularities within the disk's surface brightness distribution hint at the presence of underlying structure. Overall, the galaxy appears relatively undisturbed, with no obvious signs of a recent major merger or tidal interactions.
