The galaxy presents as a relatively compact and smooth structure. Its overall shape appears elliptical, with an estimated effective radius of roughly 4 kpc. The light distribution is centrally concentrated, exhibiting a bright, unresolved core that gradually diminishes outwards. The color profile suggests the presence of an older stellar population with a high degree of homogeneity. There may be slight asymmetries or faint tidal features suggesting a past interaction or merger event, however these features may also be artifacts. The galaxy does not show distinct spiral arms or a prominent disk-like morphology.
