The galaxy presents as a relatively smooth, elliptical structure. Its color is predominantly a yellow-orange hue, indicative of an older stellar population. The galaxy displays a moderate degree of ellipticity, appearing elongated but not highly so. No distinct spiral arms or strong dust lanes are apparent. The light distribution is concentrated towards the center, forming a bright bulge. There is a gradual decrease in light intensity moving outwards from the galactic center, fading into the background. The galaxy exhibits no obvious signs of a major merger or significant tidal disturbances. Faint hints of a disk-like feature could possibly be present, but the galaxy appears to be relatively featureless.
