The galaxy presents a generally elliptical morphology with a bright, concentrated central bulge. A fainter, more diffuse halo surrounds the central region. The light distribution appears uneven and asymmetric with some visual disturbances. There is a hint of a possible tidal tail or plume extending from the main body on one side. The overall color profile suggests a higher concentration of older stellar populations within the bulge, and bluer, younger star formation is observed in the surrounding disk or disturbed regions. This implies that the galaxy may have experienced recent or ongoing interactions or mergers that triggered enhanced star formation, disrupting the existing stellar distribution. 
