The galaxy presents as a somewhat elongated, diffuse object with a concentrated central region, exhibiting a yellowish-white hue. Its overall shape suggests a deviation from perfect circularity, leaning towards a prolate or cigar-like morphology. Indications of tidal disturbances or potential merging activity are present, with a secondary concentration of light appearing separated from the main body by a fainter bridge of light. The galaxy is characterized by an apparently smooth texture, lacking prominent spiral arm structures or distinct dust lanes in the resolution available. The light profile gradually decreases from the central concentration outwards, implying a diminishing density of stars or emitting material towards the galaxy's periphery. The object displays an intermediate color profile as well.
