The galaxy presents as a somewhat smooth, elliptical structure with an apparent cigar shape. It is centrally concentrated, exhibiting a bright, yellowish core which likely indicates an older stellar population. The galaxy gradually fades from the core outwards, transitioning into a fainter, bluish halo. This halo suggests a minor component of younger, bluer stars at the galaxy's periphery. There appear to be no significant spiral arm structures or dust lanes visible. The overall morphology suggests a galaxy that is not actively undergoing major mergers, appearing relatively undisturbed, but with a hint of possible recent or ongoing minor interactions contributing to its shape and outer star formation.
