This galaxy presents a predominantly smooth morphology. The central region exhibits a bright, concentrated bulge, appearing nearly spherical in shape. The surrounding disk shows a subtle elongation. There is a suggestion of a slight disturbance in the disk structure on the left side of the galaxy. It's color appears slightly more yellow, suggesting an older stellar population. Star formation rate for this galaxy appears low. The galaxy presents an intermediate shape, neither perfectly round nor significantly elongated, but somewhere in between. There is no clear evidence of ongoing major merger activity, though a minor disturbance cannot be ruled out.
