The galaxy presents as a relatively smooth, elliptical-like object. The core exhibits a bright, concentrated yellowish-white hue, suggesting an older stellar population. This core is surrounded by a more diffuse, lower-intensity halo. The overall shape appears somewhat elongated but not highly flattened, trending toward a spheroidal morphology. There is no apparent evidence of spiral arms, bars, or significant dust lanes. No signs of on-going or recent mergers are readily apparent. Based on the color profile, star formation is likely suppressed or minimal in this system.
