The galaxy presents as a relatively smooth, elliptical structure with a dominant central bulge. The core exhibits a concentrated luminosity, indicative of a high stellar density. The overall color profile suggests an older stellar population, with a yellow-orange hue more pronounced in the central regions. A subtle disk-like structure is potentially present but not very prominent. Possible signs of past or ongoing star formation are present in the faint greenish color at the outskirts, but seem to be weak. The shape appears generally round, with no obvious signs of major mergers or significant tidal disturbances. No distinct spiral arm structures are observed.
