The galaxy appears as an elliptical or lenticular system at a redshift of approximately 0.31. It is characterized by a dominant, centrally concentrated bulge component. The object displays a generally smooth morphology, with only subtle indications of any internal structure or spiral arms.

The galaxy exhibits a relatively compact size, with an estimated effective radius of approximately 11 kpc. Its color profile indicates a population of older stars, primarily observed in the redder bands. There are some indications of a few blue regions of star formation, though overall star formation activity is minimal.

The shape of the system is somewhat oblate, with a moderate degree of ellipticity, not appearing to be particularly round. There is no significant evidence of tidal features or ongoing mergers, suggesting that the galaxy has likely undergone a period of relative quiescence in recent times. The galaxy is fairly isolated from other objects.
