The galaxy presents a generally smooth morphology, with a high degree of central concentration. It appears relatively round, exhibiting minimal elongation. There is faint evidence of a possible minor disturbance in the structure, potentially indicative of a past or ongoing interaction. The galaxy's color profile suggests a dominant stellar population that emits strongly in the green, and red bands, giving it a yellow appearance. This suggests that the galaxy likely has an older stellar population, and a relatively low current star formation rate. There's also potential evidence suggesting it is a fairly massive galaxy.
