The galaxy presents a predominantly smooth morphology, characterized by a central bulge that appears largely spheroidal. A faint disc component is potentially present, displaying a subtle elongation. There is no distinct spiral arm structure visible. The color profile indicates an older stellar population. There may be some ongoing but minimal star formation in the disk. There is no obvious indication of a major ongoing merger, although there is a slight asymmetry that could indicate some level of recent interaction or disturbance.
