The galaxy presents as a somewhat centrally concentrated object, exhibiting a bright core region. The core demonstrates a slightly elliptical morphology, suggesting some degree of inherent structure, or a potential disk viewed at an angle. The surrounding halo appears relatively diffuse, with no discernible spiral arms or prominent features indicative of a well-defined disk. The light distribution seems somewhat irregular, with a possible interaction or disturbance hinted at. The galaxy appears to be in the redder part of the spectrum.
