The observed galaxy presents an elliptical morphology, appearing as a smooth, cigar-shaped distribution of light. The core exhibits a brighter, more concentrated intensity profile, suggesting a higher stellar density. The galaxy displays a subtle color gradient, transitioning from a predominantly reddish-orange hue in the central region to a bluer tint towards the outer edges. The absence of clearly defined spiral arms or dust lanes indicates a relatively low ongoing star formation rate. No major disturbances from merging are observed.
