The galaxy presents as a largely smooth, elliptical morphology, with a concentrated central bulge. The color profile suggests a population of older stars, exhibiting a redder hue in the core and a more muted, greenish-yellow tinge in the surrounding halo. There is minimal evidence of spiral arm structure or significant dust lanes. The overall symmetry indicates a relatively relaxed state, devoid of any major ongoing merger activity, although subtle peripheral disturbances cannot be ruled out. The luminosity appears relatively consistent across the galaxy, showing a lack of bright, concentrated star-forming regions. The structure appears mostly spheroidal, without strong elongation.
