This galaxy appears to be a relatively undisturbed system. The light is concentrated in a central bulge, transitioning smoothly outwards with diminishing intensity. The morphology appears largely elliptical, lacking any clear spiral arm structures or prominent disk features. There may be hints of a very faint halo surrounding the primary body of the galaxy, though this is difficult to ascertain due to the resolution. The overall color gradient suggests an older stellar population, with a general redder hue.
