The galaxy presents as a relatively compact object. It exhibits a primarily smooth morphology, with a central concentration of light. There is a subtle, diffuse extension or plume emanating from the central region, displaying a slightly bluer color than the main body of the galaxy. This may indicate a region of younger stars or possible tidal interactions. The main body of the galaxy appears to have a redder color, which may suggest an older stellar population. The core shows a higher surface brightness. There might be evidence of minor disturbances in the galaxy's shape, possibly indicating an ongoing or past merger event. Further investigation is needed to determine the nature and extent of the plume and assess the presence and impact of any merger activity on the overall structure and evolution of this galaxy.
