The galaxy presents a somewhat elongated, cigar-shaped morphology. Its light distribution appears relatively smooth, lacking any prominent spiral arms or defined disk structure. There is a central concentration of light, suggesting the presence of a bulge or a core region. Color gradients are subtle, but there is a general trend where the center appears whiter than the areas on the edges, implying a potential variation in stellar populations or dust content between the core and the outer regions. The galaxy shows a hint of disturbance, but overall does not seem to be undergoing a major merger event. 
