The galaxy displays a roughly elliptical morphology, with an estimated effective radius of approximately 1.8 arcseconds. The central region exhibits a smooth, concentrated light profile, with a distinct blue hue. Surrounding this core, a fainter, more diffuse halo extends outwards, appearing relatively smooth but exhibiting some irregularities in its shape and intensity. The galaxy appears to be undergoing an interaction with two neighboring objects, the larger of which is relatively smooth, but disturbed, with a green-yellow color profile and a significant, diffused tail, possibly indicating tidal disruptions. The smaller, fainter object shows similar colors to the tail of the object above it. There may be some minor merging events occurring. Overall, the galaxy displays characteristics suggestive of both an evolved stellar population within its core and ongoing or recent interactions with other galaxies.
