The galaxy presents as a centrally concentrated object with a relatively smooth morphology. It appears mostly featureless, lacking prominent spiral arms or a distinct bar structure. The core region exhibits a yellowish hue, potentially indicative of an older stellar population. The light gradually diffuses outwards from the core, transitioning to a slightly bluer tint in the outer regions. The overall shape is generally round, showing minimal elongation or asymmetry. There is no obvious sign of ongoing major mergers or strong tidal disturbances. The faintness of the outer regions suggests low star formation activity is occuring.
