The galaxy appears as an elongated structure, possibly an elliptical or a spiral galaxy seen at a significant angle. The central region displays a bright, concentrated luminosity, suggesting a dense stellar population or an active galactic nucleus. There are hints of asymmetry or disturbances in the galaxy's shape, particularly at its periphery. The color distribution shows a range of stellar populations. The central bulge exhibits a redder hue, likely indicating older, cooler stars, whereas the outer regions show bluer colors, suggesting younger, hotter stars and potentially ongoing star formation. There is a faint, diffuse halo surrounding the main body of the galaxy, implying the presence of a stellar halo or tidal debris.
