This galaxy presents as a somewhat elongated, disk-like structure. The overall color appears to be a yellowish-white, suggesting a population of older stars. There is a slight bluing toward one end which suggests the possibility of some ongoing star formation. The galaxy's smooth appearance and lack of prominent spiral arms or strong dust lanes suggest that it could be an early-type spiral or perhaps a lenticular galaxy seen at an oblique angle. There is a hint of a possible tidal disturbance or minor interaction on the right side of the disk, although more data is required to confirm such morphological peculiarity. Overall, this galaxy appears to be a moderately massive system undergoing relatively quiescent star formation.
