The galaxy presents as a single, relatively smooth object with no distinct spiral arm structures or bar. It appears elliptical in shape, with a high degree of central concentration. The light distribution is fairly uniform, showing a gradual decrease in brightness from the core outwards. The color profile suggests a dominant older stellar population, leaning towards the redder end of the spectrum in the visible light range. Minimal dust lanes or patches are observed. There are some hints of minor disturbances or tidal features, possibly indicating past or ongoing interactions, but these are subtle. The object shows no clear evidence of a strong star formation signature.
