The galaxy presents as an elongated, disk-like structure, viewed at an oblique angle to our line of sight. It exhibits a central, somewhat amorphous bulge region with a yellowish hue. The outer regions of the disk show hints of blue, possibly indicating the presence of younger stellar populations and ongoing star formation. There is some asymmetry observed in the outer disk, which could be due to a minor gravitational disturbance or tidal interaction, although no distinct merging features are immediately apparent. The galaxy appears relatively smooth overall, with limited evidence of prominent spiral arms or strong morphological features.
