The galaxy presents as a spiral type, exhibiting distinct structural features. A moderately sized bulge is apparent, characterized by a concentrated, bright, yellowish light, suggesting an older stellar population. Emanating from the central bulge are two prominent spiral arms. The winding of these arms appears relatively medium, not tightly wound nor loosely dispersed. The spiral arms display clear evidence of on-going star formation, indicated by a bluer hue relative to the bulge, suggesting the presence of younger, hotter stars. The galaxy appears to be undergoing internal structural changes.
