The galaxy presents a generally smooth morphology. It exhibits an elliptical shape, appearing more oblong than perfectly spherical. The central region is significantly brighter and more concentrated than the outer regions, suggesting a central bulge. The color profile indicates a potential mixture of stellar populations. The presence of green hints at ongoing star formation. No distinct spiral arms or significant dust lanes are visible. There is a slight asymmetry present, possibly indicating a past minor interaction or disturbance. Overall, it appears to be a relatively mature galaxy with some ongoing star formation.
