The galaxy presents a somewhat elliptical morphology. It appears relatively smooth, with a high degree of central concentration. There is a slight asymmetry evident, possibly indicating a minor interaction or internal disturbance. The galaxy's color profile suggests a population of older stars, although there might be some ongoing star formation in the central regions, given the faint blueish tinge. There is evidence of a possible tidal feature, such as a faint, extended plume or tail. High likelihood of a past or ongoing merger. The galaxy is moderately luminous, likely a spiral or elliptical with a significant stellar mass.
