The galaxy presents an elongated, cigar-shaped morphology. The central region exhibits a smooth, concentrated luminosity profile, appearing yellowish. Fainter, bluer light extends away from the central region. This suggests that the core is composed of older stars, while the outer regions may contain younger, hotter stars. There are no indications of spiral arm structures or major disturbances, appearing mostly undisturbed. Overall, the galaxy appears to be a relatively smooth system, possibly an elliptical, and its light output suggests a high mass galaxy that is no longer forming many stars.
