The galaxy appears to be an elliptical galaxy, exhibiting a generally smooth and concentrated morphology with a high degree of central light concentration. The galaxy displays a slightly elongated profile. Color gradients suggest a dominant older stellar population in the central region, as indicated by the yellowish-orange hue. There is little evidence of significant dust lanes or distinct spiral arm structures. Faint blue colors in the outer regions suggest the presence of a younger stellar population, potentially indicating a degree of ongoing or recent star formation, but at a low rate. There are no signs of any major merging events, but minor disturbances cannot be ruled out.
