The galaxy appears as a roughly elliptical object, with an estimated effective radius of approximately 8 kpc. Its color profile suggests active star formation, particularly in a concentrated region. A bluish hue is observed, indicative of the presence of young, hot stars. The galaxy exhibits a degree of disturbance, as there are no defined arms or a smooth disk and some tidal features potentially interacting nearby. The primary structure appears somewhat elongated, tending toward a cigar shape. The morphology suggests that the galaxy might be undergoing minor interactions with nearby structures, possibly a smaller companion galaxy or tidal debris. 
