The galaxy presents as a slightly elongated, cigar-shaped structure. The central region exhibits a yellowish-white hue, suggesting an older stellar population. Extending outward from the core, a blueish diffuse halo is visible, indicative of younger, hotter stars and possible ongoing star formation. The galaxy appears relatively smooth in overall structure, with no obvious spiral arms or prominent dust lanes. There are hints of some minor disturbances in the outer regions. The system appears to be in a relatively quiescent state, lacking significant merger activity or major morphological irregularities.
