The galaxy presents as a somewhat face-on or slightly inclined disk galaxy. Its color profile suggests it is a relatively mature system. The central bulge is prominent, exhibiting a smooth, concentrated light distribution. The surrounding disk shows some evidence of spiral arm structure, although it is not well-defined and appears rather flocculent. The disk itself seems relatively smooth overall, with a generally even distribution of light, but there are hints of slightly enhanced star formation regions along the spiral arms. The outer regions of the galaxy fade gently into the background sky, suggesting a well-defined edge to the luminous matter. There is no obvious evidence of a major ongoing merger or significant tidal disturbances, though some minor irregularities could indicate past interactions or internal dynamics. The color gradients suggest a mix of stellar populations, with bluer components potentially tracing younger stars in the disk and redder colors dominating the central bulge and possibly older stellar populations throughout the galaxy.
