The galaxy presents as a relatively smooth, elliptical-like structure. The core exhibits a concentrated, bright yellowish-white hue, suggesting an older stellar population. Moving outward from the core, the color transitions to a more reddish-orange, particularly along the equatorial plane, perhaps indicative of dust obscuration or regions of ongoing, albeit subdued, star formation. The galaxy appears somewhat elongated. There is no clear evidence of spiral arm structure or significant morphological disturbances, though there are minor color variations throughout the galaxy's body, and possibly a slight asymmetry on one side. Overall, the galaxy presents as a fairly mature system with a dominant bulge.
