The galaxy presents as a single, unresolved object exhibiting a generally smooth morphology. There is a subtle color gradient observable, trending from a more yellow hue in the central region to a slightly redder periphery. A small, secondary concentration of light is observed in close proximity to the central, brighter region. Overall, the object appears largely spheroidal and exhibits a high degree of central concentration. The apparent red color suggests an older stellar population and relatively low current star formation activity. There is no strong evidence of tidal features or significant morphological disturbance.
