The galaxy presents as a relatively smooth and centrally concentrated object, exhibiting an elliptical morphology. It appears slightly elongated, transitioning from a moderately rounded shape to a somewhat cigar-shaped appearance. There are suggestions of asymmetry or minor disturbances in the galaxy's structure, though not strongly indicative of an ongoing major merger event. The central region displays a brighter concentration of light, likely corresponding to the galactic bulge. A gradual color gradient is observed from the core outwards, with a transition towards redder hues, possibly indicating an older stellar population dominating the outer regions. Given the galaxy's overall characteristics, it is plausible that star formation is suppressed. The light produced is consistent with a high-mass system.
