The galaxy presents as a fairly luminous, elliptical-shaped object, exhibiting a generally smooth texture throughout its structure. The core appears to be a bright, concentrated region of older stellar populations, indicated by the yellowish hue. Moving outward from the core, the galaxy gradually fades into a less defined halo, with a color shift indicating the presence of some younger, bluer stars within the extended disk. There are no prominent spiral arms or bar structures visible; the overall morphology is more akin to a spheroid. The shape exhibits a slight elongation, indicative of a mild deviation from perfect sphericity. No signs of active galactic nuclei are obvious. The lack of major disturbances suggests a relatively stable, non-interacting system, though some minor asymmetries hint at the possibility of past or ongoing minor interactions. The object shows the characteristics of a large galaxy with little active star formation.
