This galaxy exhibits a morphology characterized primarily by a smooth, elliptical profile, though with faint, low contrast, features of an inner disk. It appears moderately luminous, with a concentrated central bulge dominating its overall light distribution. The galaxy's color gradient suggests the presence of both older stellar populations in the bulge and recent star formation within the disk.

The system does not show clear indications of a major ongoing merger, although subtle disturbances are observed. These disturbances are more likely the product of a minor interaction, internal dynamics, or past merger events. The galaxy's overall structure is neither perfectly spherical nor elongated, appearing to be between elliptical and disk galaxy.
