The galaxy presents as a face-on spiral galaxy, displaying a clear central bulge and a well-defined disk structure. The central bulge appears yellowish and exhibits a high degree of luminosity, suggesting a concentration of older stellar populations. 

Spiral arms are visible extending outwards from the central region. The spiral arms show a mottled texture, hinting at ongoing star formation regions interspersed with dust lanes. The overall color of the disk is bluer compared to the bulge, consistent with the presence of younger, hotter stars.

There is no obvious indication of significant tidal disruption or interaction with other galaxies. The disk is not perfectly smooth, suggesting some level of internal activity or minor disturbances. The morphology suggests a galaxy that is actively forming stars within its spiral arms, with an older stellar population dominating the bulge.
