The galaxy presents as a single, well-defined object. It appears to be a lenticular or elliptical galaxy, exhibiting a smooth, nearly featureless morphology with high degree of central concentration and a well-defined round shape. The color gradient suggests an aging stellar population, shifting from yellow/orange towards the center to more red hues in the outer regions. There is no evidence of spiral arm structure or prominent dust lanes. The galaxy appears undisturbed, showing no signs of ongoing major mergers or significant tidal interactions. Overall, the galaxy appears relatively quiescent, likely with suppressed star formation.
