The galaxy presents an elongated, cigar-shaped morphology. It appears relatively smooth in overall structure, lacking prominent spiral arms or a distinct central bulge. The color profile suggests a concentration of older stellar populations, with a yellow-reddish hue dominating the central regions. The outer regions exhibit a bluer tint, potentially indicating more recent, albeit subdued, star formation activity. There is no obvious indication of a major ongoing merger or significant tidal disturbance, though subtle asymmetries in the outer regions might hint at a minor interaction in its past. The galaxy appears to be a moderate-sized system, with its light output placing it between smaller dwarf galaxies and larger, more luminous systems. Overall, this galaxy appears to be a relatively quiescent system, possibly undergoing slow, steady star formation.
