The galaxy presents as an elliptical morphology with evidence of potential interaction or merging activity. Its core exhibits a high degree of spheroidal symmetry and a strong concentration of light, suggestive of an older stellar population. Extended diffuse emission is observed, possibly indicating tidal debris or disrupted galactic components. A slight asymmetry is visible in the outer regions of the galaxy, suggesting a minor disturbance. Overall, the galaxy appears to be relatively smooth in appearance, with a slight yellowish hue.
