The galaxy presents as a single, dominant, and relatively smooth structure. Its morphology appears elliptical, exhibiting a high degree of radial symmetry in its light distribution. The color gradient suggests a moderately evolved stellar population, with the central regions exhibiting a yellowish hue indicative of older stars. No distinct spiral arm structures or prominent dust lanes are discernible. The overall appearance suggests a relatively quiescent system, without substantial ongoing star formation. There are no signs of tidal disturbances or interactions with other galaxies. The light profile decreases smoothly from the center outward, implying a centrally concentrated mass distribution. The galaxy is well-defined and appears to be in a relatively relaxed state.
