The galaxy presents a largely smooth, elliptical morphology. The central region exhibits a high degree of concentration, with luminosity decreasing gradually towards the outer edges. There's a subtle elongation, suggesting a shape intermediate between perfectly round and a more cigar-like form. Evidence of spiral arms or a distinct disk structure is absent. No major mergers or significant tidal disturbances are apparent in the immediate vicinity of the galaxy. The overall colour is indicative of an older stellar population with relatively low ongoing star formation. Minor disturbances can be seen around the core.
