The galaxy appears to be undergoing a significant gravitational interaction, possibly a merger. A central, somewhat amorphous bulge of older stars is visible, exhibiting a yellowish hue. Emanating from this bulge is what appears to be a tidal tail, displaying a bluer color, indicative of younger stellar populations and ongoing star formation within the disturbed material. The overall shape suggests a distorted disk or irregular morphology, deviating significantly from a well-defined spiral or elliptical structure. There is evidence of considerable star formation activity, particularly noticeable within the tail. The galaxy is moderately luminous, suggesting a substantial stellar mass.
