The galaxy presents as a relatively compact structure. It appears to be somewhat spheroidal, with a hint of disk-like morphology. There is some indication of a more diffuse outer region. Color gradients within the galaxy suggest varying stellar populations. A bluer, possibly younger stellar population is concentrated in a portion of the galaxy, indicating ongoing or recent star formation. The remaining color is more indicative of an older population, with a smooth appearance suggesting the absence of significant dust lanes. There is no obvious sign of any tidal disturbances or ongoing major merger events.
