The galaxy presents as a spiral galaxy with a notably large, moderate-sized bulge, as indicated by the concentration of light towards the center. Two distinct spiral arms emanate from the central bulge. The spiral arms are tightly wound and feature a relatively consistent structure. The galaxy's disk appears to have a slight inclination relative to our line of sight. The color profile suggests the presence of both older stellar populations in the bulge, exhibiting yellower hues, and younger, bluer stellar populations distributed throughout the spiral arms. No significant bar structure is apparent across the disk. The galaxy appears relatively undisturbed, with no significant signs of any major merging events or strong tidal interactions with neighboring galaxies.
