The galaxy presents as an elongated structure with a moderately smooth appearance. There may be a hint of a spiral structure, but not sharply defined. The central region is brighter and more concentrated, with a relatively diffuse halo. The color appears to be more blueish in areas surrounding the central core, but with an overall reddish hue, possibly indicating the presence of both older stellar populations and ongoing star formation. The shape is moderately elongated. Based on the asymmetry, it is possible that it is undergoing a minor interaction.
