The galaxy presents as a relatively smooth and centrally concentrated light distribution. There is a slight deviation from perfect circularity; it exhibits an in-between shape, neither perfectly round nor elongated. There appears to be some sort of ongoing merger or interaction, given what can be seen here, either minor or involving multiple galaxies. Color gradients indicate a possible change in stellar populations from the core outwards, going from what appears to be a yellow center, towards a redder exterior. Despite a lack of readily-discernable spiral arms or defined structures, subtle deviations in the light profile may suggest underlying features. There is a notable radial brightness gradient, concentrated towards the central region.
