The galaxy presents as an elliptical morphology with a smooth, featureless appearance. The central region exhibits a concentrated luminosity profile, indicative of a prominent galactic nucleus. Moving outwards, the light gradually diminishes with no apparent spiral arms or distinct substructures visible. Color gradients are subtle, with a general trend towards redder hues in the central bulge and slightly bluer tones in the outer regions. The overall round shape suggests minimal rotational support. There is no apparent interaction with other galaxies or signs of recent merger events. The galaxy exhibits a redder color, suggesting it may consist of an older population of stars with little to no active star formation.
