The galaxy presents an elliptical morphology, although some disturbances are apparent. A bright, centrally concentrated bulge region is visible, displaying a yellowish-orange hue, suggestive of an older stellar population. A fainter, bluer extension emanates from this central bulge. The asymmetry and bluer color implies ongoing star formation, possibly triggered by a merger or tidal interaction. The overall light distribution is relatively smooth, however the features imply potential interaction with another galaxy or recent minor merger event.
