The galaxy presents as a single, centrally concentrated object with a generally smooth morphology. The core region exhibits a bright, yellowish-white color, indicative of a likely older stellar population. Surrounding the core is a more diffuse halo of bluish-white light that extends outwards, suggesting the presence of younger, hotter stars or some ongoing star formation within the galaxy. There is no apparent spiral structure or significant dust lane obscuration visible. The galaxy appears to be fairly isolated with no obvious signs of interaction or merging events, although a slight asymmetry in the outer halo is observed. The object has an approximate extent of 10" across.
