The galaxy presents an elliptical morphology, appearing elongated with an approximate axis ratio of 5:1. The central bulge exhibits a bright, yellowish-white hue, indicative of an older stellar population. The light distribution appears smooth, with a gradual decrease in intensity moving outwards from the core, suggesting a lack of prominent spiral arm structures. Fainter, blueish tinges along the outer edges may indicate some star formation occurring, although it is not prevalent. There are no obvious signs of tidal tails or major disturbances, suggesting the galaxy is relatively undisturbed.
