The galaxy appears as a flattened spheroid, exhibiting a smooth morphology. Its color gradient suggests a possible concentration of older stellar populations in the central regions, trending toward bluer hues in the outer parts. There is no strong evidence of spiral arm structure or a prominent central bulge. The galaxy appears relatively undisturbed with a lack of tidal tails or obvious signs of a major merger event. There may be evidence of a minor interaction with a nearby object.
