The galaxy presents as a face-on spiral galaxy with a moderately sized bulge. A bar may be present but not prominently. The spiral arms are well-defined and extend outwards from the central bulge, showing evidence of active star formation. The bluer color of the outer arms indicates a higher concentration of younger, hotter stars. There is no evidence of a major merger; however, there may be minor disturbances due to a faint companion galaxy. Overall, this galaxy exhibits a well-defined structure with ongoing star formation activity within its spiral arms.
