This galaxy exhibits an elongated, flattened morphology, characteristic of a disk galaxy viewed at an oblique angle. The central region displays a pronounced bulge, appearing yellowish-white, suggesting a population of older stars. Progressing outwards from the core, the disk shows a bluer hue, indicative of ongoing star formation, although no distinct spiral arm structure is readily discernible in this image. The overall appearance suggests a galaxy with a substantial, well-established stellar population within the bulge, with more recent star formation occurring within the disk. The light distribution appears fairly smooth, though some faint disturbances may be present. The galaxy does not show obvious signs of a major ongoing merger.
