The galaxy presents as a moderately elliptical system. Its morphology appears relatively smooth, suggesting a well-mixed stellar population. The galaxy exhibits a color gradient, with a central region that appears more yellow-white, gradually transitioning to a bluer hue towards the outer edges. This potentially indicates older stars concentrated in the core and younger, bluer stars in the disk or spiral arms. There is no clear evidence of a spiral structure. The disk has only minor disturbances. Overall, it appears to be a disk galaxy with a relatively calm or slowly-evolving morphology.
