The galaxy presents an overall smooth morphology, with a centrally concentrated light profile. The light distribution suggests an elliptical shape, tending towards round, but with some apparent elongation. The central region appears brighter and more condensed. There is some suggestion of a minor disturbance in the galaxy’s overall structure. A faint blue hue suggests the presence of some ongoing star formation, albeit at a low level. Overall, the galaxy seems to be in a relatively late stage of its evolution, potentially transitioning towards quiescence.
