The galaxy presents a predominantly smooth morphology, appearing largely featureless in this observation. Its overall shape approximates a spheroid, exhibiting a moderate degree of roundness without significant elongation. There is little evidence of distinct spiral arms or a well-defined disk structure. 

The galaxy displays a color gradient, transitioning from a brighter, yellowish-white central region to a bluer periphery. This color distribution suggests a possible difference in stellar populations, with potentially older stars concentrated towards the center and younger, bluer stars more prevalent in the outer regions.

There is no visible sign of ongoing major mergers or significant tidal disturbances. Minor asymmetries or subtle irregularities in the outer regions cannot be entirely ruled out, though these are not clearly evident. The overall light distribution is relatively concentrated, indicating a substantial central mass concentration.
