The galaxy presents a generally smooth appearance, with a concentrated central region exhibiting a bright, yellowish-orange hue. This core fades outward, transitioning into a slightly elongated and less defined halo of similar color. While the main body of the galaxy lacks distinct spiral arm structures, there are subtle irregularities in the light distribution suggesting minor disturbances or potential merging activity in its past. The roundness of the galaxy is notable, although some elongation is present, deviating from a perfect circular form. The overall color suggests an older stellar population.
