The galaxy presents as a somewhat smooth, concentrated light source with a slight elongation, possibly indicative of a disk-like structure viewed at an oblique angle. The central region appears to be dominated by an older stellar population, exhibiting a yellowish-orange hue which suggest minimal on-going star formation. A small redder area is seen on one side of the central region, possibly indicating a region of dust obscuration or a population of redder stars. Overall the galaxy does not show any distinct spiral arm structures or significant tidal disturbances, implying it has not undergone a major merger recently.
