The galaxy presents an overall elliptical morphology, appearing elongated with a high degree of cigar-shapedness. The light distribution is largely smooth, indicating an older stellar population. There is a suggestion of some subtle internal structure. A central bulge is visible with a yellow-orange hue, which is indicative of older, cooler stars. Fainter, bluer light is evident in the outer regions which suggests some degree of recent or ongoing star formation, although the dominant stellar population is likely older. There is no obvious spiral structure or prominent dust lanes. The galaxy does not display any signs of major interactions, such as tidal tails or distorted morphology, but there is a hint of minor disturbance based on the slight asymmetry in the isophotes.
