The galaxy presents as a moderately luminous, elliptical-like structure at a redshift of approximately 0.23. It exhibits a centrally concentrated brightness profile, with the light intensity decreasing gradually towards the outer regions. The core appears smooth and featureless with a golden hue, indicative of an older stellar population. The outer halo is less defined. There is only slight evidence of any significant ongoing star formation. There is no clear evidence of significant merger activity or tidal disturbances in the immediate vicinity. The galaxy is relatively isolated. It has a moderate mass.
