The galaxy presents as a relatively smooth, elliptical or lenticular structure. Its core exhibits a concentration of yellowish light, possibly indicating an older stellar population. Moving outward from the center, a gradual transition to a bluer hue can be observed, potentially suggesting the presence of some younger stars or ongoing star formation, although at a low rate. The galaxy's overall shape appears close to round, showing minimal signs of significant disturbance or tidal interactions. No distinct spiral arms or prominent dust lanes are readily apparent, supporting the assessment of it being a smooth system. Faint extensions or a slight halo might be present, but further investigation would be needed to confirm.
