The galaxy exhibits a largely smooth morphology, with a slight ellipticity in its overall shape. The light profile is centrally concentrated, displaying a bright core that gradually diminishes outwards. There is a distinct radial color gradient, transitioning from a yellowish-white center to a more reddish hue in the outer regions. This suggests an older stellar population dominates in the central bulge, with relatively lower levels of ongoing star formation. No prominent spiral arms or significant dust lanes are discernible, which coupled with its relatively smooth appearance, points towards a later-type galaxy. There is a subtle hint of faint, extended halo surrounding the main body of the galaxy.
