The galaxy presents a generally smooth morphology, exhibiting a spheroidal shape that is observed to be fairly round. There is a concentrated central bulge with a luminosity gradient that fades into a more diffuse halo. Overall, the galaxy displays a dominant color gradient, transitioning from a yellowish-orange core to a redder hue towards the outer regions, suggesting an older stellar population with little ongoing star formation. There is no obvious indication of spiral arm structures or significant dust lanes within this galaxy. Interactions or merging activity is not apparent.
