The galaxy presents an elongated, cigar-shaped morphology, suggesting an elliptical classification. Its central region exhibits a brighter, more concentrated luminosity, indicative of a prominent galactic nucleus or bulge. The galaxy appears relatively smooth in structure, lacking distinct spiral arms or prominent dust lanes. Color gradients are subtle, with the core exhibiting a slightly yellower hue compared to the outer regions, potentially due to an older stellar population. There is a slight hint of possible tidal disturbance visible. Overall, the galaxy appears to be a relatively quiescent system, potentially undergoing minimal current star formation.
