The galaxy presents as a relatively smooth, elliptical-like structure. Its overall form is elongated, exhibiting a cigar-like shape rather than perfect circular symmetry. The central region is the brightest, with luminosity gradually decreasing outwards toward the edges. There is a notable lack of distinct spiral arms or a prominent disk. Instead, the light distribution appears diffuse and homogenous throughout the galaxy's body. Some minor asymmetry or subtle irregularities exist in its outer regions, which could imply a gravitational interaction of some sort. The galaxy is colored generally white, but with some cooler tones as one looks outward from the center of the galaxy. The light produced by the galaxy appears to be relatively homogenous.
