The galaxy presents as a somewhat amorphous structure, appearing more smooth than having defined spiral arms. There may be a slight central bulge, displaying a yellowish hue, implying an older stellar population concentrated towards the center. Extending outwards from this core is a fainter, more diffuse halo of bluish light, suggesting a younger stellar population and ongoing star formation. The edges of the galaxy gradually fade into the background, with no sharp boundaries, indicating a smooth distribution of stars. There is evidence of some minor gravitational disturbance.
