The observed galaxy appears to be a spiral galaxy exhibiting a prominent bar structure that spans a considerable portion of its central region. Distinct spiral arms emanate from the ends of the bar, though they are somewhat tightly wound and display flocculent characteristics. The central bulge of the galaxy is of moderate size, contributing significantly to the galaxy's overall luminosity. There is no visible evidence of any major ongoing merger events or significant tidal disturbances, though minor irregularities might be present in the outer regions of the disk. The disk component is the dominant visual feature, appearing face-on with a clear, although somewhat diffused, spiral pattern. Overall, the galaxy presents as a well-defined spiral morphology, with the bar being the most striking characteristic.
