The galaxy presents a morphology that appears to be disturbed, possibly indicating a recent or ongoing interaction. While there is a somewhat centrally concentrated bright region, the overall structure lacks the smooth profile of a typical elliptical galaxy. This central region displays a bright white core, surrounded by a more diffuse blue emission.

The blue color suggests the presence of younger stellar populations and/or active star formation. There appears to be a slight asymmetry in the galaxy's shape, with some faint extensions or tidal features visible, again potentially indicative of an interaction. While not a clear spiral structure, there is a slight suggestion of a flattened disk-like component to the galaxy. There is no strong evidence of a major ongoing merger.
