The galaxy presents a morphology exhibiting characteristics of both smooth and featured structures. A central bulge is evident, appearing smooth and concentrated, with a yellowish-orange hue suggesting a population of older stars. Fainter, bluish features extending from the central region hint at the presence of spiral arms, although they are not well-defined. There appears to be some irregularity in the distribution of light within the disk, possibly indicating minor gravitational disturbances or interactions. The galaxy does not appear to be a late stage merger, although some disturbances are clearly present. The size of this galaxy is significant, and it appears massive. Star formation is present within the galaxy, but appears subdued.
