This galaxy exhibits an irregular morphology, with an observed axial ratio suggesting a non-spherical, elongated form. It shows evidence of a potential ongoing or recent merger event. Distinct luminous regions are visible, indicating possible tidal tails or other interaction remnants between two galaxies. The overall color profile implies a mix of stellar populations, with the brightest region being a yellow/orange hue. This hue may suggest a presence of older stars, dust obscuration, or a combination of both. Other color profiles are present with blueish hues, this may indicate regions of more active star formation. Given the irregularity and disturbed structure, this galaxy is a likely candidate for further investigation into its merger history and star formation activity.
