The galaxy presents a generally smooth morphology. The central region exhibits a high degree of luminosity, appearing almost uniformly bright. The overall shape approximates an ellipse, with a major axis roughly twice the length of its minor axis, appearing nearly round. Faint, diffuse light extends outward from the central region, indicating a surrounding halo or disk component, though no distinct spiral arms or other prominent features are discernible. The galaxy is observed to have a distinct color gradient, with the core exhibiting a bluer hue, transitioning towards redder tones at its periphery. The image suggests a possible interaction or merger with a smaller, more compact object positioned off-center. This secondary object displays a markedly redder color, perhaps indicating an older stellar population or significant dust obscuration. There is evidence of tidal distortion or disturbance in the main galaxy's outer regions. The light distribution shows no obvious signs of a barred structure or a strong central bulge, although the resolution limits a conclusive determination.
