The galaxy presents as an elliptical or lenticular type, appearing relatively smooth and featureless in this image. The central region exhibits a brighter, concentrated core, suggesting a substantial stellar population. There is a slight elongation to the galaxy's overall shape, rather than a perfect sphere. Evidence of a disk is uncertain.

A faint, diffuse halo surrounds the central region, gradually fading into the background sky. There's a subtle color gradient observed, with a slightly bluer tint in the outer regions, potentially indicating younger stars or ongoing star formation at the galactic edges. The galaxy shows evidence of minor disturbances as it does not appear to be perfectly uniform or symmetrical. The galaxy appears to be relatively compact.
