The galaxy presents a generally smooth, elliptical morphology, appearing largely spheroidal with a high degree of central concentration. The light profile decreases consistently from the core outward, indicating a lack of prominent spiral arms or a significant disk component. The color distribution appears somewhat uniform with a central region with less red light and more blue. There are no obvious signs of strong tidal interactions or ongoing major mergers, although subtle irregularities in the outer regions are evident. There may be some minor disturbances, potentially indicative of past interactions. These outer faint irregularities appear more blue. This galaxy likely has a low rate of star formation.
