The galaxy presents as a generally smooth, elliptical morphology with a prominent central bulge. The light is concentrated towards the center, indicating a higher stellar density in the core region. A faint, diffuse halo or envelope surrounds the central region, gradually fading into the background sky. There is no visible spiral arm structure or significant dust lane obscuration apparent in this image. The color appears to be mostly yellow-white, possibly indicative of an older stellar population dominating the light output. There's a slight indication of bluer light surrounding the core, which might point to a younger stellar population that is present, but not dominating the light of the object. The galaxy does not show any clear signs of recent major merger events or significant tidal distortions.
