The observed galaxy presents as a somewhat elliptical, centrally concentrated light distribution. The core region exhibits a bright, yellow-orange hue. The intensity of light decreases with radial distance from the core. At about half the distance from the center to the outer limits, the galaxy color shifts to a pale, less concentrated yellow. There appears to be a subtle tidal tail or disruption extending from the main body. The overall shape suggests a classification leaning towards an elliptical galaxy with some irregularities, possibly indicating a minor interaction or past merger event.
