The galaxy presents as a moderately sized, elliptical structure. It appears predominantly smooth in morphology, with a high degree of central concentration, likely dominated by an older stellar population in the core. The overall color gradient shows a bluer hue in the outer regions that suggest recent star formation exists. The galaxy shape tends more toward being an intermediate ellipticity. There is no apparent major disturbance of the galaxy's structure, suggesting it is not currently undergoing a major merger event. However, some faint asymmetry or minor disturbances might exist and could suggest potential past interactions with other galaxies.
