The galaxy presents an elongated morphology. Its central region exhibits a yellowish hue, suggesting a population of older stars. The outer regions display a slightly bluer tint, which could indicate the presence of younger stars or ongoing star formation, however, the overall color is more red than blue. The galaxy shows some level of disturbance within its structure, perhaps indicative of an interaction or merger. There is no definitive, regular spiral structure to observe, nor is it a perfect elliptical. There seems to be a lack of clear central bulge. Its general shape can be described as lenticular or possibly even irregular.
