The galaxy presents a predominantly smooth morphology, with a high degree of central concentration. It appears nearly round, exhibiting minimal deviation from a circular shape. The primary color component is a yellow-orange hue, suggesting an older stellar population. A slight extension or plume of bluer material emanates from the main body, potentially indicating a region of more recent star formation or a tidal feature. The overall structure does not show any prominent spiral arms or other disk-like features. There is a slight hint of irregularity in the outer isophotes, but no evidence of a major ongoing merger or significant tidal disruption.
