The observed galaxy presents as a spiral galaxy, oriented approximately face-on from our vantage point. A prominent central bulge is visible, exhibiting a yellow-white color suggesting an older stellar population. Fainter spiral arms extend outwards from the central bulge, showing a bluer color indicative of ongoing star formation. The arms exhibit some patchiness. The galaxy appears relatively isolated, with no obvious signs of tidal interactions or major mergers. There is a slight asymmetry in the shape of the arms, though no substantial disturbance. Dust lanes are subtly visible within the spiral arms. Overall, the galaxy is characterized by moderate bulge dominance and moderately-defined spiral arm structure.
