The galaxy appears to be a relatively bright, elliptical galaxy at a redshift of z=0.122, indicating substantial distance. It exhibits a flattened, cigar-like shape rather than a perfectly circular form. The galaxy's light distribution suggests a smooth, continuous structure with no distinct spiral arms or prominent dust lanes visible in this imaging. There is a color gradient, with the central region appearing yellowish-white, indicating an older stellar population, and the outer regions showing a hint of bluer light. The image does not suggest any ongoing major mergers, though some minor disturbance cannot be ruled out. The half-light radius, measuring approximately 2.7 kpc, would be considered moderate size for a galaxy of this type. The estimated stellar mass is significant, and the estimated low star formation rate classifies it as quiescent.
