The galaxy presents as a relatively smooth, centrally concentrated object. The light profile appears brightest at the core, gradually diminishing in intensity outwards. The morphology suggests a general elliptical shape, appearing mostly round with a slight deviation towards a more elongated form. There is faint evidence of a possible disk-like component, but this is not well-defined. No distinct spiral arms or bar structures are discernible. The galaxy exhibits a mixed color profile, with a yellowish-white core transitioning to a more greenish-blue hue in the outer regions. There is no clear indication of major merging activity, though there may be some subtle disturbances in the outer halo.
