The galaxy presents as an elliptical or lenticular type, exhibiting a largely smooth, featureless morphology. It appears relatively round. The galaxy's core is intensely luminous, displaying a yellow-orange hue, indicative of an older stellar population dominating the central regions. Moving outward from the core, the luminosity gradually diminishes. There may be some disk-like structure, but if so it is subtle. The galaxy's overall color profile suggests a population dominated by older, redder stars, though some bluer areas may exist, hinting at regions of ongoing, but low, star formation. There is no significant sign of tidal distortion or strong interactions with other galaxies.
