The galaxy presents a generally smooth and elliptical morphology. Its overall shape is largely spheroidal, appearing quite round. A central bulge is clearly visible, exhibiting a concentrated luminosity gradient, and dominating the galaxy's light distribution. The galaxy's color suggests an older stellar population, potentially with limited ongoing star formation. Evidence of spiral arm structures or significant dust lanes is not apparent. There are no obvious signs of recent major merger activity or strong tidal disturbances. The galaxy displays a relatively homogenous structure throughout, with only subtle variations in color and brightness observed within its main body.
