The galaxy presents as a smooth, elliptical-like structure with a slight elongation, suggestive of a cigar shape. The core appears bright and concentrated, exhibiting a yellow-orange hue that transitions to a redder color at the edges. This color gradient implies an older stellar population predominating within the galactic center, giving way to younger, hotter stars as you move outwards along its edge. There are no obvious spiral arm structures, though the possibility of a disk component cannot be ruled out. The morphology suggests that it is likely in its later stage of evolution. There are some indications of minor disturbances, possibly related to interactions with another object, but it appears overall undisturbed.
