The galaxy presents as a generally diffuse object. A concentration of light emanates from a central region, suggesting the presence of a galactic nucleus. The body of the galaxy appears disturbed, with asymmetry in the distribution of its light and matter. There is evidence of potential tidal features or debris, indicating a possible interaction with another galaxy. The color distribution is uneven, with some regions showing a shift towards shorter wavelengths. This may indicate areas of active star formation within the galaxy, but could also be due to dust obscuration. The galaxy does not exhibit a clear spiral structure or elliptical shape, suggesting it may be an irregular type. Further investigation into the galaxy's radial velocity and spectral properties will be needed to further classify this galaxy.
