The galaxy presents as a relatively smooth, elliptical or lenticular structure, appearing mostly featureless in this image. There is a distinct concentration of light towards the center, suggesting a prominent bulge. The galaxy displays a moderate degree of ellipticity, leaning towards a less rounded shape, but is not particularly elongated. Color gradients suggest a population of older stars dominating the bulge and inner regions, transitioning to slightly bluer hues in the outer parts, implying some level of ongoing, albeit low, star formation activity. There are no obvious signs of recent or ongoing major merger events or significant tidal disturbances affecting the overall morphology.
