The galaxy presents an elliptical morphology, exhibiting a smooth and largely featureless structure. The central bulge is prominent, displaying a bright and concentrated luminosity. The light distribution gradually diminishes outwards from the core, fading into the surrounding space. The galaxy's shape is noticeably elongated, with a cigar-like appearance. Evidence suggests a minimal presence of spiral arms or other distinct disk-like features. There are no signs of a major ongoing merger or significant tidal disturbances, although a faint, minor irregularity or disturbance in the outer regions may be present. The galaxy demonstrates colors consistent with an evolved stellar population.
