The galaxy presents as a somewhat elongated structure, with a pronounced central bulge exhibiting a bright, diffuse glow, suggesting a high concentration of stars in the nucleus. The outer regions of the galaxy appear less defined and more amorphous, with a cigar-like shape. There is evidence of a faint disk component with a blue-ish tint, but it is not particularly well-defined or prominent. The overall morphology points towards a galaxy undergoing active star formation, albeit at a modest rate. The galaxy does not appear to be undergoing any major mergers or disturbances, though minor disturbances are likely present.
