The galaxy presents as a moderately bright, elliptical-shaped object with a centrally concentrated luminosity profile. Its color appears relatively uniform across its extent, with a hint of bluer tones, suggesting a population of young stars mixed within an older population. There is no apparent spiral structure, nor is there any obvious dust lane obscuration or tidal tail indicative of a recent major merger event, although minor disturbances cannot be ruled out. The galaxy exhibits a smooth, slightly flattened profile, leaning towards "in-between" in terms of roundness, with no obvious strong morphological features.
