The galaxy presents as a slightly elliptical, yellowish central bulge, surrounded by a fainter and more diffuse halo. There is a possible faint disk structure or arm extending from the main body. The galaxy appears relatively smooth, with a high degree of central concentration, and a smaller object is connected to the galaxy. It is difficult to ascertain a definite structure due to the image resolution. The redshift indicates a considerable distance, influencing the apparent magnitude. Based on the color indices and overall morphology, it seems the galaxy is composed of older stars. There may be some evidence of minor disturbances, potentially indicating a past or ongoing interaction. There is a potential merging event occurring with the smaller object.
