The galaxy appears as a centrally concentrated object with a relatively smooth morphology. The light is dominated by a yellow-white core, suggestive of an older stellar population. There is a subtle gradation of light intensity outwards from the center, indicating a diffuse halo or envelope surrounding the core, with traces of bluish light. The galaxy's shape appears more in-between or intermediate than round. There is no obvious indication of prominent spiral arms, a significant disk component, or major disturbances, which could suggest the absence of recent major mergers or interactions. There is no apparent dust lane. The lack of distinct features and the overall color profile indicate that it may be an early-type galaxy.
