The galaxy presents as a moderately bright, elliptical form. A prominent central bulge is observed, appearing a yellow-orange hue, indicating an older stellar population. Moving outwards from the core, the color shifts subtly towards green, suggesting the presence of some younger, hotter stars and perhaps a small degree of on-going star formation within a disc component. The overall structure appears relatively undisturbed, with no obvious signs of a major ongoing merger or tidal disruptions. There is faint, diffuse light extending beyond the main body of the galaxy, which could be a halo of stars. The lack of distinct spiral arms or other prominent features suggests a classification leaning toward an elliptical or lenticular morphology.
