The galaxy presents as a centrally concentrated, luminous object with a smooth and largely featureless morphology. The galaxy exhibits a roughly elliptical shape, though it appears closer to an in-between circularity rather than a highly elongated, cigar-like form. The core exhibits a yellowish hue suggesting an older stellar population and/or significant dust obscuration within that region. The outer regions display a subtle color gradient, transitioning towards a redder tone, possibly indicating a gradual decrease in younger stars towards the galaxy's periphery. There is no visually apparent evidence of strong tidal interactions, merging activity, or significant spiral arm structures.
