The galaxy presents as a smooth, centrally concentrated light distribution, suggesting an elliptical morphology. The core region exhibits a bright, yellowish-white hue, potentially indicating an older stellar population dominating the galactic center. The overall shape is generally round. Fainter, greenish tinges are present in the outer regions, which could be indicative of ongoing, albeit low-level, star formation activity or the presence of a less dominant population of younger, bluer stars. There is no apparent spiral structure, bar, or signs of significant recent interaction or major disturbance to the main body of the galaxy.
