The galaxy presents as a relatively smooth, elliptical object. Its core exhibits a concentrated, bright yellowish-orange hue, suggesting a population of older stars and potentially dust obscuration. The color gradient transitions outward to a fainter, slightly bluer halo, indicating a less densely packed stellar population and possible regions of recent star formation. There is a slight asymmetry in the outer regions, though no obvious spiral arm structure or major disturbances are apparent. The galaxy's overall shape appears mostly regular, with a slight elongation along one axis, though it is generally between round and cigar shaped. Based on these features, it is likely a massive galaxy with low star formation.
