The galaxy presents as a relatively smooth, centrally concentrated object. Its overall morphology appears elliptical, exhibiting a slight elongation. The core region is the brightest, with light diminishing gradually outwards. A subtle disk-like structure might be present, but it is not clearly defined. The light appears more blue/white, indicating moderate to low levels of ongoing star formation. There is no evidence of significant dust lanes or prominent spiral arms. Some minor disturbance may be present in the outer region, although the resolution limits detailed assessment. The object is unlikely to be undergoing a major merger.