The galaxy presents as a moderately luminous object with a somewhat indistinct morphology. It appears predominantly smooth in structure, with a central concentration of light suggesting a bulge. The overall shape is elliptical, appearing more elongated than circular. The light distribution suggests a relatively evolved stellar population, with a dominant red-yellow hue. There is a faint and diffuse extension of light emanating from the central region, possibly indicating tidal features or a disrupted disk. Subtle irregularities in the outer regions might indicate minor disturbances. No clear spiral arms or prominent dust lanes are discernible. There is a potential for ongoing minor merging events, and the object appears to be in an intermediate stage between a fully relaxed elliptical and a galaxy experiencing tidal interactions.
