The galaxy presents as a somewhat elongated, luminous structure. Its morphology appears largely smooth and featureless with a higher concentration of light towards the center. There is a radial decrease in luminosity from the central core outwards. The galaxy's color profile suggests an older stellar population, with a predominantly yellow hue. The overall shape suggests an elliptical galaxy viewed from an angle, potentially a highly inclined disk galaxy without readily apparent spiral arm structures. There is no indication of active merging or significant tidal disturbances, though there might be minor asymmetry.
