The galaxy presents as a spiral structure, exhibiting a moderate bulge component that contributes significantly to its overall luminosity. Faint but visible spiral arms emanate from the central region. These arms appear somewhat tightly wound with hints of flocculent sections, suggesting a grand design spiral with moderate star formation. The galaxy displays a relatively bright central region, likely indicating the presence of an active galactic nucleus or a dense concentration of stars. The outer regions of the galaxy exhibit a bluer hue, indicative of younger stellar populations and ongoing star formation within the spiral arms. There's a possible sign of minor disturbance within the disk indicating a past merger or tidal interaction. No strong bar structure is obvious.
