The galaxy presents as a single, somewhat diffuse object with a bright, concentrated central region. There is a slight elongation visible, suggesting a flattened or disk-like structure, although the overall appearance is predominantly smooth. The core exhibits a bluer hue, potentially indicative of younger stellar populations or active star formation within the nuclear region. Fainter, redder emissions are seen in the outer regions, hinting at older stars in the surrounding galactic environment. There's a minor asymmetrical feature possibly indicative of a minor disturbance. Overall, it presents as a galaxy with a dominant smooth morphology.
