The galaxy presents a distinctly elongated, cigar-shaped morphology. Its color profile indicates a reddish or yellowish hue, suggesting a population of older stars and a relatively quiescent state of star formation. While there's a general smoothness to its appearance, subtle variations in light distribution suggest the potential presence of internal structures, possibly a faint disk component. The galaxy exhibits no obvious signs of major merger activity or significant tidal disturbances in this image, although subtle distortions could be present upon closer inspection. The observed structure is generally smooth and centrally concentrated, indicating a system that is likely well past the peak of its star formation history.
