The galaxy presents as a relatively smooth, elliptical-like structure with a bright, concentrated central bulge. The light distribution is centrally peaked, with a rapid decrease in surface brightness moving outwards from the core. There is a slight elongation, suggesting a departure from a perfectly circular morphology. The galaxy exhibits a subtle color gradient, with a bluer hue in the central regions possibly indicating ongoing or recent star formation, and appears redder toward the outer edges implying an older stellar population. There is a faint and irregular shape suggesting minor disturbances but no obvious merging events.
