This galaxy exhibits an overall elliptical morphology, appearing elongated with a noticeable cigar-shaped profile. The light distribution suggests a smooth structure, dominated by an extended bulge component with little evidence of spiral arms or distinct features. The central region appears yellowish-white, indicating a possible population of older stars, while the outer regions show a faint blueish halo, potentially hinting at some recent star formation activity in the galactic disk. The galaxy shows no obvious signs of major mergers or significant tidal disturbances, however there does appear to be a small amount of uneven structure. This suggests there may be a minor disturbance occurring, such as a dwarf galaxy merger. The central bulge exhibits a higher concentration of light, which gradually fades into the outer disk, indicating a smooth stellar density gradient within the galaxy.
