This galaxy exhibits a morphology consistent with an elliptical galaxy, but displays some features suggesting a possible disk component. Its overall shape is elongated. The central bulge is quite pronounced and exhibits a yellowish color, indicative of an older stellar population. Moving outward from the bulge, there's a fainter, bluer halo suggesting more recent, albeit subdued, star formation. The galaxy does not appear perfectly smooth; there may be some minor disturbances present that might suggest a previous or ongoing minor merger event. These disturbances are not major, as the overall structure remains largely coherent. The galaxy is intermediate in roundness, meaning it is neither perfectly spherical nor highly elongated.
