The galaxy presents as a relatively smooth, elliptical-like structure. It appears largely featureless with a concentrated central bulge, exhibiting a diffuse luminosity gradient outwards, with no immediately apparent spiral arm structures or distinct star-forming regions. The color profile suggests a general lack of recent star formation; based on the redder hue. There appears to be no signs of any major ongoing mergers, though a slight asymmetry could indicate a minor past interaction or a minor disturbance in its structure. The galaxy is generally round and lacks any significant elongation.
