The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a centrally concentrated luminosity profile, appearing nearly spheroidal with slight elongation. The color gradients suggest a redder core, indicative of an older stellar population and/or dust obscuration, surrounded by a bluer halo, possibly associated with younger stars at a distance. There is no evidence of prominent spiral arms or significant tidal features, suggesting a relaxed system without recent major mergers. A faint outer halo is discernible, blending into the background sky level. The galaxy is observed at a redshift value consistent with it being at a moderate cosmological distance.
