The galaxy appears as a centrally concentrated, moderately sized object with a generally smooth morphology. The light distribution suggests a spheroidal shape, with a significant fraction of its luminosity concentrated in the core region. The galaxy exhibits a color gradient, appearing slightly redder towards the center and becoming bluer towards the outer regions. There is little evidence of strong spiral arm structure or prominent dust lanes. The overall appearance is consistent with an elliptical or lenticular galaxy at intermediate redshift. There is no evidence of tidal tails or major distortions that would suggest recent or ongoing major merger activity.
