The observed galaxy appears to be a spiral galaxy, viewed at a slight angle relative to face-on. The galaxy exhibits a central bulge with a moderate size and a disk component where spiral arms may be present but difficult to discern. The galaxy's colour suggests a mix of stellar populations, with regions possibly containing relatively young, hot stars, and other regions containing older, cooler stars. There are indications of ongoing or recent star formation within the galaxy. There is no apparent bar structure. No major mergers are visible and any disturbance seems minor. The estimated size would make it a dwarf galaxy. 
