The galaxy exhibits an overall elliptical morphology, appearing as a flattened spheroid. Its central region is characterized by a bright, concentrated core, indicative of a substantial bulge component. This core gradually fades outwards, transitioning into a smoother halo.

There is evidence of a disk structure, with indications of spiral arms present, albeit weakly defined. The galaxy presents a slight inclination relative to our line of sight, allowing for a partial view of its internal disk. The primary color composition appears to be reddish-yellow, which could suggest a population of older stars. There is no obvious dust lane. The galaxy appears to be isolated, with no immediate signs of tidal disturbances or ongoing merger activity.
