The galaxy presents a largely smooth, elliptical morphology. Its color appears to be relatively uniform across its extent, trending towards the redder end of the spectrum. There is no prominent disk structure visible. There are no distinct spiral arms, bar features, or significant dust lanes apparent. The light is concentrated towards the center, and the isophotes appear mostly round, with no major disturbances or signs of an ongoing merger. There's a hint of a very slight extension on one side. Based on the color, the galaxy is likely composed primarily of older stellar populations, indicating a relatively low current star formation rate.
