The galaxy presents as an intermediate morphology, potentially a spiral galaxy viewed at a slight angle, or possibly an elliptical galaxy exhibiting some structural features. A bright central bulge dominates the core, emitting strongly in the yellow-green wavelengths, suggesting a significant population of older stars. Extending outwards from the bulge are fainter, blue-tinged regions, indicative of more recent star formation within a disk-like structure. 

There appears to be some minor disturbance to the galaxy's overall symmetry. This could be suggestive of minor tidal interactions, but the effect is subtle. A larger degree of disturbance would likely indicate a more intense, perhaps even major, interaction or merger.
