The galaxy presents as a lenticular or possibly an elliptical system, exhibiting a smooth, diffuse morphology with no distinct spiral arm structure visible. The object has a generally elongated, cigar-like shape. Its luminosity profile appears centrally concentrated, with the brightest region near the core gently fading outwards. The color appears to be a somewhat homogenous, indicative of an older stellar population, although some variation may be present. There are no obvious signs of active galactic nuclei activity or significant star formation regions. The morphology is largely undisturbed with no signs of major mergers, or extreme tidal disruption.