The galaxy presents as an elliptical or lenticular type, exhibiting a relatively smooth, concentrated central bulge. The galaxy appears to be more elongated than circular, showing an intermediate ellipticity. There is no obvious spiral arm structure or bar visible. The color gradient indicates a dominance of older stellar populations, with a reddish-yellow hue concentrated in the core. Fainter, bluer regions may be present in the outer regions, suggesting some recent star formation, but these are not prominent. There is no clear evidence of a major ongoing merger or significant tidal disturbances, though subtle irregularities might suggest minor gravitational interactions. The overall morphology points towards a galaxy that has undergone significant evolution, potentially nearing the end of its star-forming phase.
