The galaxy presents a somewhat elliptical morphology. It appears to possess a central bulge region exhibiting a yellowish hue, suggesting an older stellar population. Surrounding the bulge, a fainter, bluish disk is observable. This disk-like structure indicates the presence of ongoing star formation. While the disk appears relatively smooth, there are slight asymmetries suggesting minor gravitational interactions or internal disturbances. No prominent spiral arms or a strong bar structure are discernible in this image. Based on the color profile and disk-like structure, this galaxy is likely a late-type spiral or lenticular galaxy undergoing moderate levels of star formation.
