The galaxy presents as a somewhat elongated, disk-like structure, although the resolution limits a precise morphological classification. The central bulge region appears brighter and more concentrated, with a relatively smooth light distribution. Moving outwards from the center, the disk component appears to be relatively smooth and featureless. The color gradient suggests a population of relatively young, hot stars within the disk, giving it a bluish hue. There are no obvious signs of active star formation regions like prominent HII regions or spiral arm structures visible within the disk, suggesting a relatively quiescent star formation rate. The galaxy does not show significant signs of ongoing merger activity or tidal disturbances, but may be experiencing minor disturbance. It appears to be a relatively isolated galaxy. The overall morphology suggests it may be undergoing a slow transformation.
