The galaxy presents as a slightly elongated, cigar-shaped structure. Its light profile suggests a central bulge region, with a higher concentration of light, subtly fading outwards. The galaxy appears to be a generally smooth object, with hints of a disk-like structure, but no prominent spiral arms are visible. There is a minor disturbance on the left side of the galaxy. The color gradient from the central region outward appears to transition from bluer hues at the core, suggesting active star formation, to redder tones in the outer regions.
