The galaxy presents a morphology that is likely the result of an ongoing or recent merger event. Two distinct luminous components are visible. One component exhibits a bluer hue, suggestive of a population of younger, hotter stars, and appears somewhat less concentrated. The second component displays a redder color, indicative of an older stellar population, and has a more defined, concentrated core. The overall shape is irregular, lacking a clear spiral or elliptical structure. There are hints of tidal features or distorted arms, potentially evidence of gravitational interaction.
