The galaxy presents as a generally elliptical structure, with a high degree of central concentration. The core exhibits a bright, largely featureless appearance, suggesting an older stellar population and limited active star formation within this region. The outer regions fade gradually from the central brightness, displaying a smoother texture with slight irregularities in the distribution of light, possibly indicative of past minor merger events. There is subtle evidence of faint tidal features, although they are not immediately prominent. Overall, the galaxy’s morphology suggests a classification as an elliptical galaxy with potentially some past interactions.
