The galaxy presents a somewhat diffuse appearance, exhibiting a centrally concentrated luminosity profile. It displays a primarily bluish color, hinting at the presence of a younger stellar population with on-going or recent star formation, although the rate of star formation appears relatively low based on the lack of intense blue regions. There is a subtle indication of a flattened structure, potentially suggesting a disk-like morphology. While the galaxy appears mostly undisturbed, subtle asymmetry may suggest minor gravitational interaction with another galaxy.
