The galaxy exhibits a smooth, elongated morphology, suggestive of an elliptical or lenticular galaxy. Its overall color is a composite of blue and white hues, hinting at a diverse stellar population. The central region appears brighter and more condensed, indicative of a higher stellar density, likely containing an older stellar population. The outer regions display a slightly bluer tint and are more diffuse, indicating some ongoing or recent star formation. There appears to be little to no evidence of spiral arms or strong dust lanes within the galaxy, further supporting the likelihood of it being an early-type galaxy. There are no indications of any major disturbances or mergers in its structure; the galaxy seems relatively undisturbed.
