The galaxy presents a largely smooth, elliptical morphology. It exhibits a notable concentration of luminosity towards its center, suggesting a prominent galactic nucleus. The light profile appears relatively featureless, lacking the distinct spiral arm structures or prominent dust lanes characteristic of spiral galaxies. The color is generally reddish-yellow, indicative of an older stellar population with a lower rate of ongoing star formation. There is only a minor indication of any significant tidal disturbances or ongoing merger activity, based on the overall regular shape. The galaxy shows a roughly elliptical shape but is closer to a spherical shape. It is likely at a considerable distance, given its apparent size, and is likely a massive system.