The galaxy presents an overall elliptical morphology, with a smooth, featureless appearance. It has a centrally concentrated brightness profile, with the light intensity decreasing gradually from the core. The galaxy appears elongated, with a relatively high degree of flattening. There is a subtle color gradient, with the central region exhibiting a slightly bluer hue compared to the outer regions, which are redder. The redder outer regions could indicate an older stellar population, while the bluer center might suggest more recent star formation activity. There are subtle signs of possible disturbance in the outer regions, which may suggest recent or ongoing minor interactions. The overall light distribution is well-fit by a Sersic profile.