The galaxy presents as a moderately luminous, ellipsoidal structure. The light distribution appears relatively smooth, lacking prominent spiral arms or significant dust lanes. A subtle color gradient is observable, transitioning from a central region exhibiting warmer, reddish hues to outer regions displaying cooler, bluish tones. This suggests a possible variation in stellar population ages or metallicities across the galaxy's radial profile, with older, redder stars concentrated towards the core. The overall shape is elongated, indicating a degree of flattening. No signs of ongoing major mergers or significant tidal disturbances are apparent. The observed characteristics are consistent with a galaxy of substantial mass and a relatively low current star formation rate, indicative of a system in a later stage of its evolutionary lifecycle.
