The galaxy appears to be an elliptical galaxy, exhibiting a smooth, diffuse morphology. The galaxy's shape is elongated, with an axial ratio suggesting it is viewed at a significant inclination. The core exhibits a brighter, concentrated luminosity, gradually decreasing towards the outer edges. The color profile suggests an older stellar population, dominated by redder wavelengths, with a hint of bluer light in the galaxy's inner regions, hinting at some recent star formation. There is no discernible spiral structure or prominent dust lanes. No signs of ongoing major merger events are observed, although there is a slight asymmetry which may indicate a minor interaction.
