This galaxy appears to be a relatively compact object. The core exhibits a bright, concentrated luminosity, suggestive of either a dense stellar population, an active galactic nucleus, or intense star formation. There is a clear deviation from a perfectly smooth structure with a slightly asymmetric morphology visible. There are faint features that could be indicative of tidal disturbances or interactions, potentially hinting at ongoing or past merger events. The galaxy's color gradient indicates varying stellar populations or dust distribution within the galaxy. The overall size appears to be modest. 
