The galaxy presents a clear disk morphology, viewed at a slight angle relative to face-on. Spiral arms are evident, exhibiting a tightly wound structure. The bulge appears to be of moderate size, contributing significantly to the galaxy's overall luminosity. Star formation is occurring, indicated by the presence of blue regions within the spiral arms. The winding of the spiral arms is generally tight, though some arms exhibit a more medium configuration. There are no visible signs of a strong bar structure bisecting the galactic center. The overall color index suggests a redder composition than most galaxies, with an overall population of redder stars, potentially in the bulge, and areas of on going star formation in the spiral arms. There is no evidence of a major ongoing merger. However, there could be evidence of a minor disturbance or a less severe interaction affecting the overall structure.
