The galaxy presents an overall smooth morphology, though some features are potentially present. The light distribution appears concentrated toward the center, with a noticeable color gradient from a more yellow-white core to a slightly bluer halo. The overall shape is elongated, suggesting a classification somewhere between elliptical and lenticular. There is some hint of possible tidal disturbance, though it is difficult to confirm. There may be a merging occuring. The galaxy's light profile seems indicative of a relatively old stellar population in the central region, with a younger stellar population possibly contributing to the bluer outer regions.
