The galaxy presents as an elongated, elliptical morphology. The central region exhibits a bright, concentrated luminosity with a yellowish hue, suggesting an older stellar population. Progressing outwards from the core, the light gradually diffuses, with the outer regions displaying a slightly bluer tint, hinting at more recent star formation. The overall structure appears relatively smooth with minimal discernible features or distinct spiral arms. There are no indications of active galactic nuclei or strong tidal distortions from this view. The galaxy is moderately inclined relative to our line of sight, evidenced by its elongated shape. There is very little dust apparent in this image.
