This galaxy presents as a relatively smooth, elliptical structure. The color profile suggests a population of older stars, exhibiting a yellowish to reddish hue, likely indicating a lower rate of recent star formation. The galaxy appears centrally concentrated with a bright core. There is little indication of prominent spiral arms or distinct features typically associated with younger, star-forming galaxies. No substantial tidal disturbances or signs of ongoing major merger activity are apparent. Overall, it appears to be a mature, spheroidal galaxy with a well-defined and relaxed morphology.
