This galaxy presents as a relatively face-on spiral galaxy, viewed at a moderate distance. A central bulge is visible. It appears nearly oblate, but with a slight tilt, and we observe the spiral arms beginning to form. The spiral arms are moderately wound, indicative of an intermediate type spiral galaxy. The galaxy's color is noticeably bluer in the disk regions compared to the bulge, suggesting ongoing star formation within the spiral arms. The bulge itself presents a smoother, more homogenous appearance, characteristic of an older stellar population. There are no strong signs of recent major merger activity; however, the spiral arms exhibit some irregularities, potentially suggesting minor disturbances. The galaxy appears to be in a relatively isolated environment, without any signs of strong tidal interactions with neighboring galaxies in the immediate vicinity.
