The galaxy presents as an elongated, cigar-shaped structure with a relatively smooth overall appearance. The central region exhibits a prominent reddish hue, potentially indicative of an older stellar population or significant dust obscuration. Moving outwards from the core, the color transitions towards a more greenish-yellow tint, suggesting a younger stellar population and possibly ongoing star formation. There is a slight hint of a disk-like structure. There is no obvious sign of any major mergers or tidal disturbances.
