The galaxy presents as an elliptical form, with a smooth, centrally concentrated light distribution. The core appears to be a yellow-orange hue, suggesting an older stellar population. Moving outward, a faint, blueish halo can be discerned, indicating the presence of a younger population of stars, or perhaps recent minor star forming events. There is no apparent spiral structure. The overall light profile suggests a system that is neither perfectly spherical nor highly flattened. There are slight irregularities in the outer edges of the halo, hinting at possible tidal interactions or past minor mergers. No significant dust lanes are immediately visible in the image.
