The galaxy presents an elliptical morphology, appearing elongated and cigar-shaped in the image. The central region exhibits a strong concentration of light, suggesting a substantial bulge component likely comprised of older stellar populations. The color of the central region leans towards the redder end of the spectrum, indicative of evolved stars. Extending outwards from the core, a disk-like structure is subtly visible, though it appears relatively smooth and lacks prominent spiral arm features. The overall color profile suggests a mix of stellar populations, with some bluer regions possibly indicating ongoing, albeit subdued, star formation. There is no obvious signs of a major merger event.
