The galaxy appears to be an elliptical or lenticular galaxy, exhibiting a smooth, centrally concentrated morphology. The light distribution is relatively uniform without prominent spiral arms or distinct disk features. There's a slight elongation, appearing more oval than perfectly circular. The core exhibits a yellowish hue which may suggest an older stellar population. Fainter, diffuse bluish and greenish emission surround this central region, which may be indicative of some younger star formation, or tidal debris from interactions. There is no clear indication of strong tidal interaction, although there may be a slight irregularity to the outer edges of the emission that could be evidence of minor disturbance. The galaxy doesn’t show any signs of being actively merging with another object.
