The galaxy presents as a relatively smooth and elliptical structure. Its core exhibits a strong, yellowish concentration of light, suggesting a significant population of older stars. The galaxy appears somewhat elongated, rather than perfectly spherical. The outer regions display a gradual fading in luminosity, with hints of bluer tones intermixed with the dominant yellow light, potentially indicating pockets of younger stars or ongoing star formation, although this is faint. The overall morphology suggests it is likely a galaxy that is not currently undergoing any major mergers, although there is a slight indication of disturbance.
