The galaxy presents a centrally concentrated, smooth morphology. The light profile appears to be dominated by an elliptical bulge, exhibiting a radial color gradient where the core region appears more yellow, potentially indicating a higher concentration of older stellar populations. The outer regions display a bluer hue suggesting the presence of younger stars or ongoing star formation, albeit at a low rate. The overall shape is neither perfectly spherical nor highly elongated but rather displays a moderate ellipticity. There is no obvious evidence of spiral arms or strong tidal disturbances; however, subtle asymmetries or faint features cannot be entirely ruled out due to the image resolution.
