The galaxy presents a generally smooth and rounded morphology, exhibiting a high degree of central concentration. Its light profile is largely uniform, lacking prominent spiral arms or a distinct bar structure. There are no noticeable tidal tails or other signs of recent major mergers, although some minor disturbances cannot be completely ruled out.

The color distribution suggests a relatively old stellar population, with a noticeable lack of blue star-forming regions. The dominant hues are indicative of evolved stars and a dearth of ongoing star formation. While the image resolution is limited, the overall appearance is consistent with an elliptical galaxy or a lenticular galaxy with a dominant bulge component.
