The galaxy presents as a relatively smooth, elliptical structure. It exhibits a concentrated central bulge, transitioning to a fainter, diffuse halo. The core region displays a yellowish-white hue, suggesting an older stellar population and a lack of significant ongoing star formation in the nucleus. The outer regions of the galaxy appear slightly bluer, which may indicate the presence of a younger stellar population compared to the core, though star formation appears overall low. There is no obvious evidence of spiral arm structure or a prominent dust lane. The galaxy does not show signs of tidal disturbances or ongoing merger activity, indicating a relatively quiescent state. The shape is mostly round, with a slight ellipticity.
