The galaxy appears to be a spiral galaxy, viewed approximately face-on. Two prominent spiral arms are visible, tracing a relatively tightly wound pattern around the galactic center. These arms display a mottled texture indicative of active star formation regions. The nucleus of the galaxy presents a moderate bulge, with a yellowish color suggesting an older stellar population. The overall color of the disk is bluish, consistent with a younger, hotter stellar population distributed throughout the spiral arms. The spiral arms do not appear highly disturbed, suggesting no major ongoing mergers, though some minor irregularities in their structure hint at possible past or minor interactions. The galaxy appears relatively isolated with no obvious large companions close to it. There is a hint of a bar structure bisecting the central bulge, but it is not particularly pronounced.
