The galaxy presents as a relatively compact spiral structure. The spiral arms are somewhat tightly wound, suggesting a classification towards the earlier end of the spiral sequence. While somewhat blurred, the presence of at least two to three distinct arms can be inferred. A central bulge is observable, appearing to contribute a moderate fraction to the galaxy's overall luminosity. The colors indicate a mix of stellar populations, with a yellow-ish central region indicating older stars. The galaxy is unlikely to be undergoing major mergers, although the spiral arms could be slightly disturbed due to minor interactions with nearby galaxies. Overall, it presents as a normal spiral galaxy.
