This galaxy exhibits a relatively smooth morphology with a dominant central bulge. The color profile indicates a redder core, suggesting an older stellar population is concentrated in the center. The overall shape appears somewhat elongated or cigar-shaped. No prominent spiral arms or dust lanes are visible, hinting at either a lack of recent major merger activity or a state where such features have already dissipated. There is a slight blue tint along the edges of the galaxy, which may suggest recent star formation along its periphery, but this could also be an artifact. The galaxy appears relatively undisturbed with no major signs of ongoing merger activity, but there is a possibility of minor disturbances that are difficult to resolve at this resolution.
