The galaxy appears to be a relatively smooth, elongated elliptical or lenticular type. It exhibits a centrally concentrated bulge, which appears yellowish-white in color, suggesting an older stellar population. The galaxy's overall shape is somewhat cigar-shaped, with a higher concentration of light towards the center, fading towards the edges. There is a subtle hint of a disk-like structure, but it is not well-defined. No spiral arms or significant dust lanes are visible in this image. The galaxy shows no strong signs of a major ongoing merger or significant tidal disturbances, though minor irregularities cannot be ruled out completely. The light distribution suggests a relatively evolved system with a small specific star formation rate.
