The galaxy presents as a somewhat diffuse, irregular object with a centrally concentrated luminosity. The overall color is bluish, suggesting a moderate presence of younger stellar populations. The morphology seems to be significantly disturbed, possibly indicating ongoing or recent merger activity. There appears to be evidence of tidal features or disrupted structures extending away from the main body of the galaxy, hinting at gravitational interactions. The smoothness of the overall light distribution is broken by these apparent disturbances. The galaxy exhibits an amorphous shape rather than a well-defined spiral or elliptical structure.
