The galaxy appears as a diffuse, moderately small object. It exhibits a somewhat irregular shape with a slight elongation along a single axis. The light distribution is centrally concentrated, although not perfectly symmetrical. There is evidence of a faint, blueish color, suggesting the presence of young, hot stars and regions of active star formation. The overall texture of the galaxy is relatively smooth, but subtle irregularities and faint structures may exist within its disk. Given the overall structure, color, and apparent size, it is likely a dwarf galaxy with a low mass and modest star formation rate. There are potential signs of disturbance within the central region of the galaxy, which may be indicative of a minor interaction with another nearby system.
