The galaxy presents as a spiral galaxy, exhibiting a prominent disk structure with a central bulge. The spiral arms are moderately defined, showing a relatively tight winding pattern as they emanate from the central region. Multiple spiral arms are discernible, estimated to be at least three or four. The bulge appears to be of moderate size compared to the overall disk, showing a yellow-white color, suggesting a higher concentration of older stars. Patches of bluer light are visible within the spiral arms, indicating regions of active star formation. No significant signs of a major merger event or strong tidal disturbances are observed, although there might be minor irregularities. The galaxy does not appear to be viewed edge-on.
