The galaxy presents as a centrally concentrated, smooth object. Its morphology is predominantly elliptical, exhibiting a high degree of roundness. There's a slight elongation, but it does not appear cigar-shaped. No spiral arm structures are visible, and the galaxy's light is dominated by a central bulge that fades gradually into its outer regions. No signs of major mergers or tidal disturbances are apparent; however, a possible minor disturbance is not ruled out. Color gradients suggest a relatively uniform stellar population, with a slight concentration of bluer colors toward the core, possibly indicating some ongoing star formation. The galaxy's overall appearance suggests a mature system, potentially having exhausted much of its gas and dust.
