This galaxy exhibits a generally smooth morphology, with a centrally concentrated luminosity profile. It appears somewhat rounded, deviating slightly from a perfectly circular shape. There are indications of minor disturbances in its structure, possibly resulting from interactions or internal dynamics. The overall color of the galaxy suggests an older stellar population. There is the possibility of it merging with another galaxy based on visible disturbances and color profile. The size of the galaxy appears to be within the average range observed for galaxies at its approximate redshift.
