The galaxy exhibits a generally smooth morphology, with a bright, concentrated central bulge. Some subtle features or a disk-like structure may be present, but these are not highly defined in the image. A slight degree of disturbance, possibly a minor merger or interaction, cannot be completely ruled out. The galaxy has a modest size and a colour profile suggesting intermediate redshift. A relatively strong red component suggests the presence of older stellar populations, while the presence of blue light indicates ongoing star formation. The overall light distribution appears centrally concentrated with possible extended, fainter regions around the main body of the galaxy.
