The galaxy presents as a roughly circular, smooth object with no discernible spiral arm structure or a distinct galactic bar. The light distribution is centrally concentrated, indicative of a prominent bulge. There's a color gradient visible, with a yellowish-white hue at the core, suggesting an older stellar population dominating the central region. The outer regions of the galaxy appear slightly bluer, hinting at the presence of a younger, possibly star-forming population, although this activity is likely moderate. The galaxy does not display any clear signs of tidal disturbances or ongoing major mergers. There is a slight asymmetry in the outer regions, but it is not significant enough to classify it as an actively merging system. The overall morphology suggests a galaxy that has largely completed its assembly, possibly an elliptical or an early-type spiral galaxy viewed face-on.
