The galaxy presents as a somewhat elliptical, though moderately irregular, system. The light distribution is largely smooth, with a gradual falloff in intensity from the center outwards, and a hint of a disk-like feature. There is a slight elongation, with the major axis significantly larger than the minor axis, indicating a deviation from a perfect sphere. The color profile appears relatively uniform across the galaxy's body, suggesting a population of older stars with modest ongoing star formation. Some minor disturbance is visible in the galaxy's morphology. This galaxy appears to be in a relatively isolated location, with no immediately obvious indications of major gravitational interactions with any other significant galaxies.
