The galaxy presents as a spiral type, with moderately well-defined spiral arms emanating from a central bulge. The arms appear somewhat tightly wound, displaying a relatively uniform distribution of luminosity. The galaxy exhibits a clear disk structure, which is viewed at a slight angle. The central bulge is bright and appears relatively small compared to the overall galaxy size, suggesting it is not overly dominant. There is a slight asymmetry in the distribution of light within the spiral arms which suggests a mild gravitational disturbance from interactions with nearby galaxies, however there is no sign of a complete merger. The galaxy exhibits some neutral hydrogen gas content. The color distribution suggests active star formation is present within the spiral arms, evidenced by bluer hues, with an older stellar population concentrated in the central bulge, as indicated by its yellower color. The image exhibits some degree of ellipticity, suggesting it isn't perfectly face-on.
