The galaxy presents as a largely featureless, elliptical-like structure. Its overall morphology appears smooth and well-defined. The central region exhibits a concentrated, bright core, suggestive of a significant stellar population and potentially an active galactic nucleus. Moving outward from the core, the light gradually diffuses, forming a faint halo surrounding the galaxy. 

There is a slight elongation, the overall shape is more akin to a rounded form rather than a highly elongated or cigar-shaped one. Evidence of significant disk structures, spiral arms, or other prominent features is lacking. No indications of major mergers or tidal disturbances are visible. The color profile indicates a dominance of older stellar populations. The subtle gradient from the core outwards gives some indication of the spatial distribution of the galaxy's star formation rate. From that we can determine it has a moderately suppressed star formation rate relative to its mass, implying it is a relatively passive system nearing the red sequence. 
