The galaxy presents a somewhat elliptical morphology, displaying characteristics of a relatively smooth structure. The central region exhibits a concentrated luminosity, suggesting a prominent bulge. The outer regions gradually fade, indicative of a stellar halo extending outwards. There is a subtle disk-like structure present. The galaxy displays a yellowish-red hue, potentially indicating an older stellar population with lower rates of recent star formation. No significant tidal disturbances or signs of ongoing major merger events are readily apparent in the image, although there is some slight asymmetry evident which could indicate a minor disturbance or interaction. Overall, the galaxy appears relatively undisturbed and evolved.
