The galaxy presents as a generally smooth, somewhat elliptical structure. There is a central bulge exhibiting a concentrated, bright core, emitting primarily yellowish light. The overall shape appears to be somewhere in between round and elongated. The galaxy appears to be undergoing relatively little major merging activity. The outskirts display a fainter blueish hue, suggesting a moderate presence of younger stars and ongoing or recent star formation, though the overall star formation rate appears fairly low. There may be minor disturbances in the outer disk that may indicate a minor merger.
