The object presents as an elliptical galaxy, displaying a smooth, featureless morphology. The light distribution suggests a centrally concentrated spheroid, elongated significantly along one axis. The galaxy exhibits a dominant yellowish-orange color, indicative of an older stellar population. There's no discernible spiral structure, dust lanes, or bright knots of star formation visible within the resolution limits. A slight color gradient appears, with the central region appearing more intensely yellow and a subtle fading towards the outer edges, suggesting a potential variation in stellar population or metallicity from the core outwards. There is no evidence of a recent or ongoing major merger event, though subtle asymmetry could indicate minor tidal interactions or past minor merger activity.
