The galaxy presents as a slightly inclined, lenticular structure. The central bulge appears bright and concentrated with a yellowish hue. This suggests an older stellar population with a lower rate of active star formation within the bulge region. Surrounding the bulge is a disk component that is visibly bluer in coloration compared to the bulge. This may be due to the presence of younger, hotter stars and ongoing star formation. The outer edges of the disk appear relatively smooth with no obvious signs of strong spiral arm structures or major disturbances. There's a subtle asymmetry in the disk, but the overall impression is that of a relatively undisturbed system.
