The galaxy presents as a somewhat diffuse object with a roughly elliptical morphology. The central region exhibits a brighter, more concentrated core, surrounded by a fainter, more extended halo.  The light distribution appears relatively smooth, though with some irregularities suggesting potential disturbances. The galaxy's color profile indicates a bluer hue, potentially indicative of ongoing or recent star formation. Overall, the galaxy does not show a strong disk structure, but has light that appears to be broadly flattened and more of an elliptical shape. There are hints of disruption in the galaxy's overall structure.
