The galaxy appears as a centrally concentrated object with a generally smooth morphology. It exhibits a largely spheroidal shape, with a subtle color gradient from a more reddish hue at the core to a slightly greenish tinge in the outer regions. No prominent spiral arms or significant dust lanes are discernible in this image. The overall light distribution suggests a relatively homogenous stellar population, indicative of an older system with a low ongoing star formation rate. There is no clear evidence of recent merger activity or major disturbances to its structure.
