The galaxy presents a somewhat amorphous appearance. It has an estimated effective radius of approximately 4.7 kpc, and a low star formation rate, suggesting that it is primarily composed of an older stellar population. The galaxy exhibits a moderate degree of disturbance, with evidence of a possible past or ongoing interaction, which is likely responsible for the overall irregularity in its shape. The object is not particularly well-defined, and shows signs of disruption. There may be multiple interacting components to the galaxy.
