The galaxy appears to be a relatively large, luminous system. It exhibits a generally smooth morphology, with a somewhat elliptical shape that leans toward being round. The central region displays a concentrated, bright yellowish-white light, indicative of an older stellar population or possible AGN activity. A diffuse, bluer halo surrounds the core, suggesting the presence of some younger stars, or ongoing star formation. There are faint and subtle hints of spiral structure, but nothing concrete. There seems to be little evidence of any ongoing merger activity or significant tidal disturbances. The galaxy's overall color is relatively red, which, given its estimated distance implied by its redshift of approximately 0.23, indicates a substantial population of older stars with lower star formation rates. 
