The galaxy presents as a somewhat elliptical object, exhibiting a relatively smooth, featureless morphology. Its core appears as a concentrated bright region. There's a noticeable color gradient from the center outwards. The central region has a bluish-white hue, suggesting the presence of a population of relatively young, hot stars. The outer regions show a tendency towards redder colors, possibly indicating an older stellar population and/or dust obscuration. There is some subtle evidence of slight irregularities or disturbances in the outer regions, suggesting possible past interactions or internal dynamics influencing its shape. Overall, the galaxy appears relatively isolated.
