The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. The core exhibits a bright, yellowish-white luminosity, suggestive of an older stellar population. Fainter blueish-white light diffuses outwards, giving it a more diffuse appearance around the central region, possibly indicating ongoing star formation. There appear to be no distinct spiral arm structures or other prominent features typically associated with disk galaxies, instead a generally amorphous shape appears to be present. No signs of tidal disturbances or mergers with other galaxies are visually apparent, indicating a relatively isolated and quiescent system.
