The galaxy presents as an elongated, cigar-shaped structure. The core region exhibits a concentrated, luminous intensity, appearing smooth in texture. Moving outwards from the core, the light appears to gradually dissipate. The overall color profile seems to lean towards redder wavelengths with an inner glow of green and gold, suggesting the presence of an older stellar population throughout the galaxy. There are no easily visible distinct spiral arms or prominent dust lanes. The structure appears relatively undisturbed with only a few hints of features that may have been formed through merger events.
