This galaxy exhibits a generally smooth morphology, with a high degree of central concentration. The shape is somewhat elongated, tending toward an elliptical form, though significant deviations from perfect ellipticity are present.

The color gradient indicates a possible older stellar population toward the central region, exhibiting a more yellow hue, transitioning to a slightly bluer color in the outer regions suggesting younger stars. There's little evidence of well-defined spiral arm structures or significant dust lanes within the galaxy's disk. The lack of obvious features suggests that this is likely a quiescent galaxy with limited ongoing star formation.

Some faint asymmetries, such as slight tidal disturbances, may indicate past or ongoing interaction with another galactic object but no major mergers appear to be taking place.