The galaxy presents a generally smooth, elliptical morphology, with a high degree of central concentration. The light distribution appears relatively uniform across the main body, suggesting an older stellar population. The galaxy exhibits a distinctly round shape. Evident are minor disturbances in its structure, such as a slight asymmetry in its outer regions. These perturbations suggest that the galaxy may have experienced a minor interaction or accretion event in its past. The lack of a defined disk or spiral arm structure supports a classification as an elliptical galaxy. There appears to be ongoing merging, and the presence of a single nucleus implies it is in the late stage of merging. Overall, the galaxy exhibits characteristics consistent with an elliptical galaxy that has undergone a minor interaction.
