The galaxy presents as a relatively compact object with a somewhat irregular morphology. The light distribution appears diffuse, lacking a well-defined nucleus or distinct spiral arm structures. The object displays a dominant central region of light, potentially indicative of a bulge or core, though the resolution is insufficient to determine its exact nature.

Color gradients are subtle, but the central region exhibits a slightly bluer hue in comparison to the outer regions, possibly suggesting a population of younger, hotter stars or ongoing star formation in the galaxy's core. There is a hint of slight disturbance or tidal features within the image, but they are weak. Overall, the galaxy could possibly be undergoing a minor interaction.
