The galaxy presents as a relatively smooth, elliptical or lenticular structure. It exhibits a high degree of radial symmetry, appearing mostly round in shape. There is a subtle color gradient, transitioning from a slightly bluer hue in the outer regions to a more pronounced reddish-yellow concentration towards the galaxy's core. There is a subtle suggestion of minor structural disturbance present, possibly indicative of a past or ongoing interaction or merger event. Star formation appears to be relatively quiescent based on the lack of prominent blue star-forming regions. Overall, the galaxy appears to be a massive system consisting primarily of older stellar populations.
