The galaxy presents as a disk galaxy with a clearly defined central bulge. A prominent ring structure surrounds the central bulge, showing hints of spiral arm morphology, though somewhat diffuse. The bulge appears more luminous and yellowish, indicative of an older stellar population. The ring structure exhibits a bluer hue, suggesting ongoing star formation. The galaxy appears to be at a slight angle with respect to our line of sight. Based on visual assessment, the bulge constitutes a moderate fraction of the galaxy's overall size. There is no visual evidence of any major mergers or significant disturbances to the main structure of the galaxy.
