The galaxy presents as a spiral with a prominent, moderately sized bulge. The disk component is visible, exhibiting a relatively tightly wound spiral arm structure. There seems to be at least one or two well-defined spiral arms extending from the central region. There is a slight inclination visible suggesting we don't see the disk fully face-on. The galaxy appears relatively symmetrical, without obvious major disturbances that might suggest a recent major merger event. The overall color profile suggests a mixture of stellar populations, with a yellowish central bulge potentially indicating older stars, and bluer hues in the disk possibly associated with ongoing star formation.
