The galaxy presents a generally smooth, elliptical morphology. Its shape is elongated, exhibiting an intermediate axis ratio, appearing somewhat cigar-shaped. There is a centrally concentrated region showing redder hues, potentially indicating an older stellar population or dust obscuration. The outer regions display a bluer color, suggesting the presence of younger stars or ongoing star formation, though at a relatively low rate. There is a subtle asymmetry to the overall structure, hinting at possible past interactions or minor disturbances. No distinct spiral arms or a well-defined disk component are apparent. There are no obvious signs of a major ongoing merger, though a slight irregularity in the shape may indicate a minor merging event.
