The galaxy presents as a largely featureless, elliptical-like structure. The light is concentrated towards the center, indicating a prominent galactic nucleus. The color profile suggests a higher proportion of older stellar populations, emitting light in the redder part of the spectrum, giving it a yellowish color. There appears to be little evidence of active star formation or dust lanes, contributing to its smooth, homogenous appearance. There is little to no indication of a spiral arm structure or significant ongoing merger activity. The object shows a high degree of central symmetry, reinforcing the conclusion of an elliptical or lenticular morphology. The galaxy appears isolated, with no visible signs of tidal interactions with nearby objects.
