The galaxy presents as an elliptical system with a relatively smooth morphology, though some irregularities suggest potential disturbances. A possible merging event with a smaller object is occurring, which appears as an extension of the primary galaxy along one axis. The galaxy exhibits a yellow-red color profile, indicative of an older stellar population with likely lower ongoing star formation. The core of the galaxy appears more concentrated, gradually fading outwards. The overall shape is somewhere between a circle and an elongated shape. There are indications of asymmetry within the overall light distribution which may suggest that the merger has not yet fully resolved.
