The galaxy presents a somewhat amorphous morphology, neither purely elliptical nor clearly spiral. It exhibits a dominant, centrally concentrated bulge with a yellowish-white hue, suggesting an older stellar population. There's faint evidence of a disk component, though it lacks well-defined spiral arms or structures. Some irregularities are present, potentially indicating minor gravitational disturbances or recent interactions. The overall color profile indicates a moderate level of star formation activity but not particularly intense. It has an intermediate luminosity and falls between being a disk galaxy and a elliptical.
