The galaxy presents a generally smooth morphology, suggesting an elliptical or lenticular classification. It appears approximately elliptical, with a high degree of central concentration. The color profile indicates a dominant population of older stars. The galaxy's structure lacks prominent spiral arms or a well-defined disk. There is a slight suggestion of a minor disturbance, though no clear tidal features or ongoing mergers are readily apparent in the image. The estimated size is roughly 5 kpc in radius. Star formation appears low.
