The galaxy presents as a relatively smooth, elliptical or lenticular system, exhibiting minimal discernible substructure. The light profile appears centrally concentrated, with a gradual decrease in intensity moving outward from the core. The core displays a yellowish hue, possibly indicative of an older stellar population. The outer regions of the galaxy show a subtle shift towards redder colors. No distinct spiral arms, bars, or dust lanes are observed. The overall morphology suggests a system that is relatively quiescent, with limited ongoing star formation activity. The approximate size of the galaxy spans an estimated 6-7 kpc. There is no visible evidence of any ongoing major merger events, or other large tidal disturbances.
