The galaxy presents as a diffuse, irregular object with a dominant central region and two distinct, smaller, outlying regions. The central region appears nearly spherical and exhibits a bright, concentrated core, suggesting a possible bulge or active galactic nucleus. The overall color is bluish, implying a significant population of young, hot stars and ongoing star formation. The two outlying regions are also bluish, although less intense, which may indicate regions of recent star formation. There are potential indications of a merger or tidal disturbance in the galaxy's morphology. A slight distortion or elongation is visible and there are some indications of internal structure. Based on the color profile, the galaxy seems to be actively forming stars at a moderate rate, giving it a somewhat clumpy appearance.
