The galaxy presents as a lenticular or early-type spiral. The central bulge exhibits a smooth, concentrated luminosity profile with a yellowish hue, suggesting a population of older stars. A faint, flattened disk extends outwards from the bulge, exhibiting some subtle color variations. The disk appears slightly elongated, potentially indicating an inclination relative to our line of sight. There is faint evidence of very loosely wound spiral arms, although no regions of intense star formation are immediately apparent. The overall structure is relatively smooth with no obvious signs of a major merger event or strong tidal disturbances.
