The galaxy presents an overall elliptical morphology, elongated with a cigar-like shape. Its central region exhibits a brighter, concentrated luminosity, suggesting a relatively high stellar density in the core. Moving outward, the luminosity gradually decreases, transitioning into a fainter, diffuse halo or envelope. There is a slight hint of possible disturbance or interaction with another galaxy, as indicated by some asymmetry in its structure. There is evidence of low star formation activity. The galaxy appears to be in a relatively quiescent state, displaying characteristics of a red-sequence galaxy.
