The galaxy presents as a moderately luminous, early-type system, likely an elliptical or lenticular galaxy at a redshift of approximately 0.15. It exhibits a generally smooth, centrally concentrated morphology, with a high degree of rotational symmetry. There is a slight elongation, appearing more oval than perfectly spherical. The galaxy's light profile is dominated by older stellar populations, inferred from the relatively red color indices, and with a mass around 10^10.7 solar masses. A low-level of ongoing star formation may be present. No significant signs of tidal disturbances or major mergers are immediately apparent in the image, although minor disturbances may be present. It appears to be a relatively isolated system in its local environment.
