The galaxy presents as a small, relatively faint object with a prominent, bright central core. This core exhibits a blue-green hue, suggesting the presence of younger stars and active star formation. A fainter, diffuse extension emanates from the core, trailing off in a south-westerly direction. This extension appears bluer in color than the core, possibly indicating a stellar stream or tidal tail resulting from a past interaction with another galaxy. The overall morphology seems disturbed, lacking a clear spiral structure or elliptical symmetry. It's difficult to ascertain the exact nature of the galaxy's morphology, but based on the disturbed features and the color distribution, it is likely experiencing a period of enhanced star formation, potentially triggered by a past merger event.
