The galaxy presents a smooth, elliptical morphology, with a high degree of central concentration. A bright, yellowish core dominates the light profile, suggesting a significant population of older stars in the galactic nucleus. The light gradually decreases moving outwards from the center to its edges, indicating no prominent spiral arms or distinct features within the galaxy's structure. The galaxy appears mostly smooth, possibly a result of its stage in galactic evolution, or because it is being seen at an angle that hides spiral arms if they exist. There is no indication of major mergers or tidal disturbances. The overall color of the galaxy leans towards redder wavelengths, which would typically mean there is a lack of young, blue stars, suggesting a relatively low star formation rate. The galaxy's apparent shape is somewhat elongated, hinting at a non-spherical, potentially disc-like structure viewed at an angle.
