The galaxy presents as a slightly inclined spiral, appearing more face-on than edge-on. Well defined spiral arms emanate from a central bulge region. The arms exhibit a clumpy morphology, suggestive of active star formation regions. The bulge appears relatively compact and bright. The blue hue indicates a population of relatively young, hot stars, further supporting star forming activity. There appears to be a minor interaction or tidal feature visible as a small irregular extension from one of the spiral arms. The main body of the galaxy is largely undisturbed and well defined, indicating the tidal interactions may not be that prominent or that the galaxy is in its early stages of merging. The presence of a weak bar structure cannot be ruled out, although the features are not prominent. Overall, the galaxy appears to be a spiral type with ongoing star formation and possible minor interaction.
