The galaxy presents as a somewhat elliptical object with a central, concentrated bulge that appears yellowish-white in color, suggesting an older stellar population. The outer regions of the galaxy exhibit a more diffuse, bluish hue, possibly indicating the presence of younger, hotter stars and ongoing star formation, albeit at a low rate. The galaxy has a relatively smooth appearance with no obvious spiral arm structure or distinct features. The shape is somewhat elongated but not exceptionally so, trending towards a less-flattened spheroidal form. There is no visual evidence of a major ongoing merger or tidal disturbance affecting the galaxy's structure. However, there is a possibility of minor disturbances present. Overall, the galaxy appears to be a relatively massive system at an estimated distance implied by its redshift.
