The galaxy appears as a centrally concentrated object with a smooth, elliptical morphology. The galaxy exhibits a relatively uniform color profile across its extent, trending towards redder hues, suggesting an older stellar population. There are no prominent dust lanes or spiral arm structures visible. The isophotes appear regular and well-defined, with a high degree of circularity. There is no evidence of significant tidal disturbances or ongoing merger activity in this image. Based on the red color profile and smooth morphology, it is likely an early-type galaxy, potentially an elliptical.
