The galaxy presents an elliptical morphology, appearing as a smooth, elongated spheroid. Its color gradient transitions from a yellowish-white core to a slightly bluer outer halo. There appears to be little to no discernible spiral arm structure within the resolution afforded by the image. The overall light distribution seems to be dominated by older stellar populations, which would contribute to the observed yellowish-white central color. The slight bluing towards the edges suggests pockets of modest star formation activity, although it is possible this is just because of the way color works in astronomical images. The galaxy exhibits some signs of disturbance, or perhaps there could be a minor satellite experiencing tidal disruption.
