The galaxy presents as a relatively bright object with a noticeable disk structure. It exhibits a generally smooth morphology, although some subtle features are present suggesting internal activity or minor disturbances. The color profile indicates a mix of stellar populations, with a central region that appears more yellow/red, possibly indicating older stars or dust obscuration. The outer regions show hints of bluer light, suggesting the presence of younger, hotter stars and ongoing star formation. The galaxy's shape is somewhere between a perfect circle and a cigar, appearing like a moderately elliptical disk. There is no indication of any significant ongoing merger activity, it looks relatively stable with a slight disturbance.
