The galaxy presents as a centrally concentrated object, exhibiting a generally smooth and elliptical morphology. Its color profile suggests a dominant population of older stars, with a yellowish hue permeating throughout. There is no discernible spiral arm structure or significant dust lane obscuration apparent. The overall light distribution appears quite uniform, suggesting a relaxed and evolved stellar population. The galaxy seems well-isolated with no obvious signs of ongoing or recent mergers or tidal disturbances. A gradual falloff in luminosity is observed from the core outwards, with no indication of recent star formation.
