The galaxy presents an elliptical morphology, appearing largely smooth and concentrated. The light distribution shows a radially decreasing intensity from the core. The central region exhibits a yellowish hue, which suggests a population of older stars. There are indications of possible interactions or mergers with other galaxies; the main body has minor asymmetric light distribution that can be hints of disturbance within the galaxy. Its overall structure is dominated by a smooth profile with features that indicate recent or ongoing activity.
