This galaxy appears to be an elliptical or lenticular type, presenting a smooth, diffuse morphology. The light distribution is centrally concentrated with a noticeable decrease in surface brightness moving outward from the core. There is a slight elongation with the major axis oriented in a roughly southeast to northwest direction. The core region exhibits a yellowish-white hue, suggesting an older stellar population. Surrounding the core, a more diffuse, bluish halo is observed, which may indicate the presence of some younger stars or ongoing, albeit limited, star formation activity. No distinct spiral arms or dust lanes are visible. There is no indication of a recent major merger, although the slight asymmetry could suggest minor tidal interactions or past accretion events. The overall color gradient suggests a radial distribution of stellar populations, with older stars concentrated toward the center and younger stars distributed more sparsely in the outer regions.
