The galaxy presents as a centrally concentrated, elliptical-like structure. The core exhibits a bright, yellowish hue, suggestive of an older stellar population. The light smoothly diffuses outward from the nucleus, transitioning to a slightly redder and dimmer halo. The overall form is moderately round, appearing neither perfectly spherical nor significantly elongated. There is a subtle hint of a possible minor disturbance, perhaps indicating a previous or ongoing interaction with a smaller galactic object. There is no apparent distinct disk component or spiral arm structure visible in this image.
