The galaxy presents a slightly elongated, elliptical morphology. Its central region exhibits a smooth, concentrated light distribution. The overall color appears relatively uniform with a hint of redness, suggesting a population of older stars and a relatively low ongoing star formation rate. There is a subtle suggestion of faint outer structure, possibly indicating a disk component or tidal features due to past interactions, but overall the light is dominated by the spheroidal component. There is no obvious sign of a major merger, although subtle asymmetry suggests a minor interaction in the past.