The galaxy presents as a slightly elongated, disk-shaped structure with a yellowish hue, indicative of a population of older stars and a dearth of recent star formation. The central bulge appears prominent and smoothly distributed, with the ends of the disk gradually tapering off. The overall morphology suggests an elliptical or lenticular galaxy, though a faint disk component may be present. It exhibits some characteristics indicating a relatively high stellar mass. There are no discernible spiral arms or dust lanes, which further supports the observation of a system with little ongoing star formation. The galaxy shows signs of a moderate redshift, putting its light into the redder part of the spectrum. The galaxy shows indications of being isolated, with no visible signs of a major merger.