The galaxy presents as a somewhat amorphous, elliptical structure with an apparent major axis of roughly 20 kiloparsecs, exhibiting a smooth, featureless morphology. There are no obvious spiral arms or a prominent central bulge. Color gradients suggest a slightly redder hue overall, possibly indicating an older stellar population. This is further suggested by a relatively low rate of star formation. There is an asymmetry to the galaxy's light distribution, with some indications of a potential disturbance or interaction, maybe a small tidal tail or faint bridge connecting to another object. It may be the late stage of an ongoing merger with another galaxy. There are no obvious dust lanes or regions of intense star formation visible in this image. 
