The galaxy presents a largely spheroidal morphology with a concentrated central bulge exhibiting a yellowish hue, suggestive of an older stellar population. Extending outward from the core is a more diffuse halo, showing faint blue-greenish tinges indicative of ongoing star formation. The overall structure appears relatively smooth with some minor asymmetry observed in the outer regions. The faintness and smoothness imply that this is a large galaxy at a significant distance, possibly a large elliptical galaxy. There may be slight disturbances in the galaxy, possibly from an ongoing minor merger.
