The galaxy appears as a compact, moderately bright object with a roughly elliptical morphology. It exhibits a core of intense blue light, suggesting the presence of active star formation or a luminous active galactic nucleus. Surrounding this core, fainter, elongated structures are visible that display a hint of tidal distortion. The galaxy’s light profile is mostly smooth, but there is a notable deviation from this overall smoothness, indicating the presence of some sort of disturbance. The color gradient, moving from the core outwards, suggests a population of older stars in the outer regions. There is no clear indication of spiral arms, but the disturbed morphology could potentially be attributed to a recent merger event.
