The galaxy presents as a somewhat elliptical, rather featureless structure with a bright central bulge. The light distribution appears smooth, with a high degree of central concentration. There is a subtle elongation, possibly indicating a flattened spheroidal shape or a weak disk component viewed at an oblique angle. Color gradients suggest an older stellar population dominating the central bulge, while the fainter, bluer outer regions hint at ongoing, though perhaps modest, star formation. No significant dust lanes, spiral arms, or tidal features are apparent in this image, indicating a relatively undisturbed system. The overall appearance is consistent with an intermediate-mass galaxy, likely an early-type spiral or elliptical.
