The galaxy presents as a fairly smooth, elliptical structure with a bright, concentrated core that transitions gradually into a more diffuse halo. The color profile suggests a redder central region, potentially indicating an older stellar population or higher dust concentration. Moving outward from the core, there is a subtle shift toward bluer hues, possibly indicative of younger stars beginning to form in the outer regions. No distinct spiral arm structures or prominent dust lanes are discernible. The overall morphology suggests a galaxy that is well-evolved and has a significant stellar mass. There is no indication of ongoing major merger activity or strong tidal disturbances, implying a relatively isolated system or one that has already completed a merger process.
