The galaxy appears as a disk-shaped structure, presented at an oblique angle relative to our line of sight. Its overall color is yellowish-white, suggesting an older stellar population. The galaxy's light distribution is centrally concentrated, with a bright, relatively smooth bulge region, indicating a high degree of symmetry.

The outer regions of the galaxy seem to exhibit some degree of disturbance, possibly subtle tidal features or indications of minor interactions. No distinct spiral arm structure is discernible. The lack of prominent blue regions or bright knots of emission suggests a relatively low current star formation rate within the galaxy.
