The galaxy presents as a relatively compact, elliptical morphology with a smooth light distribution. There is a noticeable concentration of light towards the galactic center, indicative of a significant bulge component. The overall color appears yellowish-orange, suggesting an older stellar population, and a potential lack of recent star formation. No distinct spiral arms or prominent dust lanes are visible within the galaxy's structure. There's a subtle elongation, but the galaxy appears generally spheroidal. A slight irregularity is observed, potentially indicative of a minor gravitational interaction or internal instability, although no significant tidal features or merging companions are apparent. The galaxy exhibits a high degree of central concentration.
