The galaxy presents as a disk-shaped structure with a noticeable inclination relative to our line of sight. The central region exhibits a high surface brightness concentration of light, suggesting a bulge component. Surrounding this central region, a fainter, more diffuse disk is observed. The disk shows some signs of internal structure. There is a smooth component to the structure, but there are signs that it has undergone interactions. The overall color of the galaxy is generally redder in the central region, transitioning to slightly bluer hues in the outer disk. This color gradient may indicate variations in stellar populations and dust content across the galaxy. There is little sign of spiral arms or merging activity, though there are some possible hints of disturbances in its shape. The apparent diameter is approximately 4 arcseconds.
