The galaxy presents as a somewhat elliptical, smooth object. It exhibits a concentrated central bulge, appearing as a bright, yellowish core. A more diffuse, fainter halo surrounds the core. The halo exhibits a subtle color gradient, fading from yellowish-green closer to the core to a faint bluish hue further out. No distinct spiral arms or prominent dust lanes are readily visible. The overall structure suggests a lack of significant ongoing star formation, with a smooth morphology indicative of an older stellar population. There is a suggestion of minor disturbances in the outer halo, perhaps tidal features, although they are not sharply defined. The rounded appearance of the galaxy indicates a minimal rotational velocity.
