The galaxy presents as a centrally concentrated elliptical or lenticular type. The morphology is largely smooth and featureless, lacking discernible spiral arms or a prominent disk structure. The overall shape is nearly circular. The color gradient suggests an older stellar population with a yellowish-red hue concentrated towards the galactic center, possibly indicating a higher density of evolved stars in the core. The outer regions exhibit a slightly bluer color, hinting at a younger, though likely still suppressed, star formation rate. There is no visual evidence of ongoing major mergers or significant tidal disturbances. Small features are present but do not indicate if they are part of the host galaxy or artifacts.
