The galaxy presents as a centrally concentrated object with a generally smooth morphology. There is no clear spiral arm structure visible. The light distribution appears roughly circular, with a slight deviation towards an elongated shape. Color gradients suggest a relatively homogeneous stellar population, with bluer colors concentrated in the central region, possibly indicating ongoing star formation. There is no obvious dust lane or significant morphological disturbance suggestive of a recent major merger, although a subtle asymmetry hints at possible minor tidal interactions. The object has an estimated size of approximately 4 kiloparsecs. Based on the color and overall structure, the galaxy appears to be an early-type spiral or possibly a lenticular galaxy.
