The galaxy presents a somewhat irregular morphology. A dominant, centrally concentrated component exhibits a bluish hue, suggesting the presence of a younger stellar population and ongoing star formation. To the left is a yellower component, perhaps an indication of an older stellar population, or dust obscuration. There is a faint indication of asymmetry or tidal features emanating from the main body, possibly indicating a past or ongoing interaction. The galaxy appears relatively compact, with an estimated effective radius of approximately 5 kpc. Its absolute magnitude indicates that it is a dwarf galaxy. Overall, the galaxy presents a complex structure, possibly resulting from a recent merger or tidal interaction. The estimated stellar mass of the galaxy is within the range of 10^9 solar masses. Low levels of star formation are ongoing.
