The galaxy presents a relatively smooth morphology, with a centrally concentrated bulge that dominates the overall structure. The light distribution appears elliptical, with a high degree of central concentration. There are indications of a faint, extended halo or disk component surrounding the central bulge, although it appears relatively featureless and blended. The galaxy's color gradient suggests that the central regions are dominated by older stellar populations, indicated by the yellowish hue, while the outer regions may contain younger, bluer stars, though the overall color appears relatively red. There is no clear evidence of strong spiral arms or other prominent features typically associated with actively star-forming disk galaxies. There are hints of slight disturbances in the morphology, but nothing to suggest a major merger event is taking place. The lack of well-defined spiral arms or distinct features suggests this could be a lenticular or an elliptical galaxy.
