The galaxy presents as a face-on spiral with a defined structure. A bright, concentrated central bulge emits a yellowish light, indicative of an older stellar population. Two prominent spiral arms emerge from the central region, tracing a relatively well-defined path as they extend outwards. The arms are speckled with regions of bluer light, suggestive of ongoing star formation. The outer regions of the disk appear somewhat flocculent, possibly due to tidal interactions. A small companion galaxy is visible nearby. The overall color of the galaxy is moderately blue-tinged, which implies the presence of active star formation.
