The galaxy appears as an elliptical system, exhibiting a generally smooth and rounded morphology. Its color profile suggests a dominant population of older stars, presenting a yellowish-red hue concentrated towards the galactic center. There is minimal evidence of spiral arm structures or significant dust lanes. The galaxy appears relatively undisturbed, showing no prominent signs of ongoing merger activity or tidal distortions, with no distinct features that suggest recent interactions. The overall structure indicates a high degree of central concentration, typical of early-type galaxies, with a luminosity profile that fades gradually into the background sky.
