The galaxy presents as a single, relatively compact object with a smooth, centrally concentrated light profile. It exhibits a slightly elongated morphology, appearing somewhat oval or cigar-shaped, rather than perfectly circular. The object is predominantly bluish in color, particularly in its central regions, suggesting the presence of a younger stellar population and ongoing star formation. There is a subtle fading in brightness from the core outward. The overall structure appears undisturbed, without any obvious signs of major mergers or significant tidal interactions. A minor asymmetry or possible minor disturbance is suspected in the outer regions of the galaxy. 
