The galaxy presents as a relatively bright object with a defined core. The central region exhibits a yellowish hue, potentially indicating a population of older stars. Surrounding this core is a more diffuse, less concentrated area with a bluer tint. This may suggest regions of ongoing or recent star formation. The overall shape is elongated, appearing somewhere in between a circular and highly elongated shape. There is a hint of possible disruption or interaction, with what appears to be a somewhat distorted outer halo, possibly due to a minor disturbance. The morphology can be classified as a disk galaxy, or even a lenticular galaxy.
