The galaxy presents a generally smooth morphology. The central region exhibits a bright, concentrated core, fading outwards to a more diffuse halo. Its overall shape is elongated, appearing somewhat cigar-shaped rather than perfectly spherical. There is no obvious indication of spiral arms or distinct disk-like structures. The color profile suggests a population of older stars, with a reddish-yellow hue dominating the galaxy's overall appearance. Subtle irregularities or disturbances may be present, but they are not visually prominent, suggesting no major ongoing merging events or tidal interactions. 
