The galaxy appears as a relatively smooth, elliptical-like structure. It is centrally concentrated with a bright core, suggesting a high stellar density in the nucleus. There is a color gradient, with the central region exhibiting a yellowish hue, possibly indicative of an older stellar population. Fainter, more diffuse light extends outwards, gradually fading into the background. Subtle irregular features appear at the periphery, potentially indicating minor disturbances or interactions. There may be slight asymmetries or irregularities in the outer halo region, but overall, the galaxy maintains a generally regular form.
