The galaxy presents an overall elliptical morphology, although it is not perfectly symmetrical. It exhibits a central bulge region which appears brighter and more concentrated. There is evidence of an extended disk, less well defined. The galaxy shows color variation, with a redder hue in the central bulge indicating a population of older stars. Faint and distorted arms or tidal features suggest a possible interaction or past merger event. There seems to be a smaller companion object near the edge of the galaxy.
