The galaxy presents as an elliptical or lenticular type, exhibiting a largely smooth morphology with a near-round overall shape. There is little to no visible disk structure or spiral arm features. The light is concentrated toward the center, displaying a bright, concentrated core. There might be a slight color gradient, with the central regions appearing more yellowish, suggesting an older stellar population and lower star formation rate in the core, transitioning to a slightly bluer hue in the outer regions. There do not appear to be any major disturbances or signs of recent merger activity, as the galaxy's structure seems relatively undisturbed and symmetrical. The galaxy's overall color indicates a mid-range redshift, which is consistent with the presence of an older population of stars within.
