The galaxy appears as a relatively smooth, elliptical-like structure. The light distribution is centrally concentrated, exhibiting a radial gradient in brightness that decreases outwards from the core. The color profile suggests a somewhat redder population of stars. This indicates an older stellar population, potentially with lower ongoing star formation. There are subtle irregularities in its shape, giving the impression of an object that is "in-between" elliptical and disk-like. No prominent spiral arm structures, bars, or dust lanes are distinctly visible. There is the possibility of a minor disturbance to its shape, possibly a slight tidal interaction or minor merger event in the past.
