The galaxy presents as a relatively small, elongated structure. Its light profile is smooth, with a diffuse and amorphous appearance, lacking prominent spiral arms or a distinct central bulge. The galaxy exhibits a bluish hue, suggesting the presence of a population of young, hot stars, which may indicate ongoing, though potentially weak, star formation activity. The galaxy does not appear to be significantly disturbed or interacting with other galaxies, based on the lack of tidal tails or other obvious signs of gravitational interaction. The overall morphology suggests a late-type dwarf galaxy, possibly a dwarf irregular or a transitioning dwarf spheroidal galaxy. The general color and smooth structure suggest a system that has largely exhausted its gas reservoir and is either quiescent or experiencing a low level of star formation.
