The galaxy presents as an elliptical morphology, elongated along a defined axis. The light distribution suggests a high degree of central concentration, appearing relatively smooth and featureless. The core region exhibits a bright, concentrated luminosity that gradually fades toward the outer edges. There is a subtle color gradient, with the core appearing to have a slightly yellower or redder hue compared to the bluer outer regions. This subtle color variation may indicate variations in stellar population or dust content across the galaxy. The galaxy's overall structure appears undisturbed, exhibiting no major signs of tidal interactions or mergers.
