The galaxy presents as a generally smooth, elliptical structure. The core appears bright and concentrated, with a diffuse halo extending outwards. The galaxy exhibits a slight elongation, deviating from a perfect circular form. There is a subtle color gradient visible, transitioning from a yellowish hue at the core to a redder tone in the outer regions. This color gradient may suggest an older stellar population dominating the central region, with relatively less recent star formation occurring there. Faint features, possibly indicative of minor disturbances or tidal interactions, are observed in the surrounding regions. These may be indicative of past or ongoing interactions. Overall, the galaxy appears to be a massive system.
