The galaxy presents as an elongated, elliptical morphology. Its light is dominated by a central, bright region, suggesting a substantial concentration of older stellar populations. This core appears yellowish, indicative of evolved stars. Surrounding the core is a more diffuse envelope, with some hint of bluer regions intermixed. The overall structure seems relatively smooth, lacking the prominent spiral arms or irregular features associated with actively star-forming galaxies or recent major mergers. There might be a slight distortion in its shape, hinting at a possible minor interaction or disturbance, but further data would be required to confirm this. The galaxy shows evidence of ongoing, albeit relatively subdued, star formation.
