The galaxy presents an overall elliptical morphology, appearing elongated along its major axis. The central bulge exhibits a bright, concentrated luminosity profile, suggesting a high stellar density, likely comprised of older stellar populations. The disk component, while present, appears relatively smooth and exhibits a less prominent star-forming region compared to typical spiral galaxies. There are hints of minor disturbances in its structure, indicative of possible past interactions or mergers. The galaxy appears to be undergoing some star formation. The color distribution suggests a population mix, with the central bulge displaying a yellowish hue and the outer disk regions showing a bluer tint.
