The galaxy presents a prominent disk structure with well-defined spiral arms. These arms exhibit a relatively open morphology, suggesting ongoing star formation. Some patchy regions of bluer light are observed along the spiral arms, indicative of active star-forming regions. The central bulge appears to be moderately sized and has a more yellow or red coloration compared to the disk, potentially signaling an older stellar population. The galaxy's overall light distribution indicates a fairly high rate of star formation relative to its stellar mass. There are minor disturbances noted, possibly caused by an interaction, though the galaxy does not appear to be in a major merger. The disk is not edge-on. A stellar bar is present, but does not appear very strong.