The galaxy presents an overall elliptical morphology. It exhibits a smooth light profile, concentrated towards the center, with a gradual decrease in luminosity outwards. The color distribution appears relatively uniform, displaying a general yellowish-orange hue across its structure. No distinct spiral arms or prominent dust lanes are discernible in the image. The galaxy appears somewhat elongated, rather than perfectly spherical. There are no obvious signs of significant tidal disturbances or recent merger activity. The galaxy possesses a substantial mass, indicative of an evolved stellar population, but with ongoing moderate star formation. The estimated half-light radius suggests a relatively compact size.
