The galaxy presents as an elliptical morphology, lacking prominent spiral arms or a well-defined disk structure. Its overall form appears smooth and relatively featureless. There is a concentration of light towards the center, suggesting a centrally located bulge, but the light distribution decreases gradually outwards, indicating a lack of sharp edges. The color profile is primarily a yellowish hue, possibly indicating an older stellar population. There is no strong evidence of active star formation regions or significant dust lanes. The image hints at some slight asymmetry in the outer regions, which might indicate past interactions or minor disturbances, but there is no clear indication of any major ongoing merging event.
