The galaxy appears as a relatively compact, elliptical or lenticular system. It exhibits a smooth, centrally concentrated light profile, suggesting an older stellar population dominates its overall structure. There are no clear indications of spiral arms or prominent dust lanes. The color appears consistent throughout the galaxy, with a slightly yellowish hue, which supports an older, passively evolving population. It appears quite isolated, with no obvious signs of tidal disturbances or ongoing mergers with nearby galaxies. The galaxy is roughly circular in shape. There may be a very slight distortion in its morphology, but this is very minor.
