The galaxy presents as a spiral type, with a clear disk structure. Evident spiral arm formations extend from a central bulge. The spiral arms exhibit a clumpy structure, suggestive of active star formation regions. The central bulge appears moderately sized and is bright. There is no major disturbance nor presence of another galaxy nearby that would indicate a recent or ongoing merger. The galaxy is tilted relative to our line of sight, but not fully edge-on. It shows a slight hint of a bar structure within the central region. The overall color profile suggests a mix of older stellar populations in the bulge and younger, bluer stars within the spiral arms.
