The galaxy presents as a largely featureless elliptical, exhibiting a high degree of central concentration with a smooth, diffuse halo. The galaxy appears nearly round. There is little evidence of spiral arms, dust lanes, or significant tidal disturbances, suggesting it has not undergone any major mergers recently. The color profile shifts from a bluer hue towards the outer regions to a more yellowish-red core, indicative of an older stellar population dominating the central region with younger stars being in the outskirts. Overall, the galaxy appears to be a relatively quiescent system with low ongoing star formation activity.
