The galaxy presents an elliptical morphology, appearing relatively smooth and concentrated. The central region exhibits a strong concentration of light, suggesting a prominent galactic nucleus or bulge. The color profile indicates a population of older stars, with a noticeable shift toward redder wavelengths. The galaxy appears somewhat elongated along a particular axis and has a relatively compact size. The surrounding galactic halo seems faint and diffuse. There is very little evidence of active star formation, which corresponds to its redder color profile and smooth structure. There is no obvious sign of tidal disturbances, or other signs of major mergers, although minor interactions can't be ruled out. Overall, the galaxy appears to be a relatively evolved system.
