The galaxy appears to be a relatively smooth, elliptical galaxy, though the shape is somewhat elongated. The central bulge exhibits a bright, concentrated luminosity with a yellowish hue, suggesting an older stellar population. The surrounding halo displays a fainter, more diffuse light. The transition between the bulge and the halo seems gradual. Some subtle irregularities in the outer regions suggest the potential presence of minor tidal disturbances or faint spiral arms, although the overall structure is dominated by its elliptical morphology. The galaxy exhibits a slight inclination relative to our line of sight.
