The galaxy presents a predominantly smooth and elliptical morphology. It exhibits a somewhat elongated shape, appearing more akin to an oblate spheroid than a perfect sphere. The central region displays a concentrated luminosity, suggesting a substantial stellar population within the galactic nucleus. A color gradient is discernible, transitioning from a warmer hue in the core to cooler, bluish tones in the outer regions. This bluer tint implies the presence of younger stars in the outskirts, possibly indicating ongoing or recent star formation, albeit at a modest rate. There is no clear evidence of significant spiral arm structures or major disturbances from mergers. Minor irregularities are observed in the outer halo which could be signs of an older merger event, but are more likely simply areas of differing stellar density. Overall, the galaxy appears to be a relatively quiescent system, transitioning away from star formation.
