The galaxy appears to be a relatively smooth, elliptical galaxy, exhibiting a dominant central bulge with little discernible structure. It appears round, with a near-circular isophotal shape. The galaxy presents a color gradient, transitioning from a somewhat bluer hue in its central regions to redder tones in its outer reaches, suggesting a centrally concentrated population of younger stars surrounded by an older, redder stellar population. There is no obvious sign of spiral arm structure or ongoing major mergers; however, some minor disturbances may be present. Overall, the galaxy is a moderately luminous object, with a likely substantial stellar mass and a relatively low star formation rate.
