The galaxy presents a generally smooth and rounded morphology. The light distribution is concentrated towards the center, suggesting a bulge-dominated system. There's little evidence of spiral arm structure or a prominent disk. The galaxy exhibits a yellow-orange hue, potentially indicating an older stellar population with lower star formation activity and a larger proportion of evolved stars. A very minor bluer region appears to be present. There are no clear signs of any major mergers or significant tidal disturbances affecting its structure.
