The galaxy appears to be a lenticular or early-type spiral, seen at an oblique angle, and exhibiting a relatively smooth light distribution across its body. There is a slight elongation, suggesting it is not perfectly spherical and tending toward a cigar shape. The galaxy presents a dominant blue hue, with a hint of color variation, particularly in the inner regions. There is a redder area visible, perhaps a sign of a less active region or dust obscuration. There is a suggestion of a faint disk, but with no obvious spiral arms. There appear to be some minor disturbances, which could be due to gravitational interactions with another galaxy. The general appearance suggests an older stellar population with low star formation. The central region of the galaxy is brighter and more compact than the outer regions, showing a weak bulge.