The galaxy appears as an elliptical or lenticular type, exhibiting a largely smooth morphology with minimal discernible structure. The central bulge displays a yellowish hue, possibly indicative of an older stellar population. Moving outward from the core, the galactic disk fades into a bluer tint, suggesting the presence of younger, hotter stars within the extended regions. The galaxy presents with a high degree of symmetry and a degree of roundness, showing little sign of ongoing or recent major mergers. Slight irregularities in the outer regions may be the result of a minor gravitational interaction, or star formation. The overall colour suggests a galaxy undergoing moderate levels of star formation relative to its mass. The galaxy appears quite massive and luminous.
