The galaxy presents a generally smooth appearance, exhibiting a centrally concentrated luminosity profile with a slight elongation in shape. The central region displays a warmer hue, transitioning outwards to cooler tones. There is a slight visual asymmetry, as the overall form seems more developed on one side compared to the other. There is faint indication of some structural feature, although no large scale spiral arms or a well defined disc are evident, with the majority of the structure being found in the central core. There are no evident merging signatures.
