The galaxy presents a relatively smooth morphology, potentially exhibiting features of both elliptical and spiral characteristics. It appears elongated, with an estimated effective radius of approximately 6.6 kpc. The color distribution suggests an older stellar population, given the redder hue, yet potentially with ongoing star formation implied by bluer regions within the galaxy. Based on its shape, it could potentially be an edge-on disk galaxy, or a spheroidal galaxy with a flattened shape. There may be a minor interaction or disturbance in the morphology of the galaxy, but that needs further observations to confirm.
