The galaxy presents a smooth, elongated morphology. It is observed to have a central concentration of light, indicating a bulge. The color profile suggests a dominant older stellar population, with a redder hue towards the center, potentially indicating dust obscuration. Some irregular light distribution present. The overall shape is somewhat cigar-shaped. There appear to be no strong signs of spiral arm structure and/or a disk. No significant signs of tidal disturbances or ongoing major merger activity are visible.
