The galaxy presents a largely smooth and elliptical morphology, with minimal discernible substructure in this image. It exhibits a concentrated, bright central region, possibly indicative of a significant bulge component. The color profile displays a gradient from a yellowish-white core outwards to more reddish fringes, suggesting an older stellar population dominating the inner regions and comparatively younger stars residing at the outskirts. There's little to no evidence of spiral arms or prominent dust lanes from this view. The overall symmetry is undisturbed, showing no apparent signs of ongoing major mergers, although subtle disturbances cannot be ruled out at this resolution. It appears to be a quiescent galaxy, possibly a lenticular or elliptical galaxy nearing the red sequence.
