The galaxy appears to be a lenticular or early-type spiral galaxy, possibly with an elliptical component. Its light distribution suggests a smooth and centrally concentrated bulge, lacking prominent spiral arm structures. There are some minor disturbances to the light from the galaxy, which may suggest that the galaxy is in the process of merging with another galaxy. The galaxy exhibits a slight elongation, with an estimated axis ratio of approximately 0.4. The half-light radius is estimated to be around 8.6 kpc, implying a moderate size. The galaxy's color indices suggest a redder stellar population, consistent with older stars and a low star formation rate. This assessment aligns with its measured photometric redshift of approximately 0.11.
