The galaxy presents as a relatively smooth, disk-like structure with a noticeable central bulge. The bulge exhibits a yellowish-white hue, suggesting an older stellar population. The disk component appears less well-defined, displaying a mixture of green and reddish tones that are not uniformly distributed. The observed colors suggest ongoing or recent star formation regions within the disk, as well as a contribution from older stars. The galaxy appears moderately inclined to our line of sight. There is no strong evidence of a recent major merger, but there may be some signs of minor tidal disturbances, which could indicate smaller interactions.
