The galaxy appears to be a relatively compact object, exhibiting a smooth, elliptical morphology with a high degree of central concentration. The galaxy's color profile suggests a dominant population of older stars, with a redder hue indicative of lower star formation activity and a lack of prominent spiral arms or disk-like structures. There's no apparent dust lane or significant tidal disturbance, further supporting the classification as an elliptical galaxy. The overall light distribution is regular and lacks significant irregularities or features that would suggest ongoing mergers or interactions.
