The galaxy presents as a relatively smooth, disk-shaped structure with an elliptical morphology. There is a central bulge exhibiting a yellowish-orange hue, which likely indicates an older stellar population. Moving outwards from the bulge, a flattened disk structure becomes apparent, displaying a subtle blue-ish tint. This bluer coloration suggests the presence of younger, hotter stars in the disk. There are no distinct spiral arm structures visible in this image; however, the color variations do show a disk-like arrangement of stars and dust. The galaxy appears to be undisturbed, without any obvious signs of recent major mergers or interactions, with a moderate degree of rotational symmetry. The object appears relatively isolated in this field of view. 
