The galaxy presents an overall elliptical morphology, appearing elongated with a cigar-like shape. The central region exhibits a concentration of light, suggesting a prominent galactic nucleus. Fainter, diffuse light extends outwards from the core, indicating the presence of a stellar halo or disk. Based on the color indices, the galaxy appears to have a moderate amount of ongoing star formation, although it's not extremely high. No signs of major disturbances or ongoing merging events are visually apparent; however, there are subtle features that could indicate minor disturbances. The galaxy is relatively smooth in overall texture. The effective radius suggests that the galaxy is relatively compact.
