The galaxy presents as a somewhat elliptical object, exhibiting a smooth, diffuse morphology. The primary concentration of light suggests a prominent central bulge, potentially indicative of an older stellar population. There's a slight asymmetry to the galactic structure, showing some evidence of a disk-like component. The color gradient transitions from a bluer hue at one edge to a warmer yellow near the center, hinting at spatial variations in stellar populations and/or dust content. While the overall structure appears relatively undisturbed, there might be subtle signs of minor tidal interactions, possibly with a faint companion.
