The galaxy presents a generally smooth appearance, exhibiting a centrally concentrated luminosity profile. The morphology is largely elliptical, appearing mostly round. There is an indication of a slight elongation, but it is not pronounced. The galaxy's color gradient suggests that the core region contains an older stellar population exhibiting redder hues, fading to a very subtle greenish hue in the outer regions, possibly indicating younger stars or some ongoing, albeit low, star formation. There are no obvious signs of recent mergers or major disturbances in the galaxy's structure.
