The galaxy presents a generally elliptical morphology with a concentrated, luminous core. The light distribution appears smooth, with a lack of apparent spiral arm structures or significant dust lanes. The central region exhibits a yellow-orange hue, indicative of an older stellar population, potentially dominated by red giant stars. There is a subtle color gradient from the core outwards, with the outer regions displaying a slightly bluer tint, possibly suggesting the presence of younger stars in these areas, though overall star formation appears suppressed. The galaxy exhibits no obvious signs of ongoing major mergers or tidal interactions with nearby objects. Minor disturbances may be present.
