The galaxy presents a concentrated central bulge, appearing nearly spherical in shape. The bulge exhibits a yellowish-white hue, suggesting a population of older stars. A faint, diffuse disk surrounds the central bulge. This disk is not well-defined and exhibits hints of bluer light, possibly indicative of ongoing or recent star formation. The overall structure implies an elliptical morphology, although some disk-like characteristics are present. There may be a minor disturbance or interaction occurring. A fainter component is visible, potentially involved in a tidal interaction or merger event.
