The galaxy presents a flattened, elliptical morphology. It is characterized by a bright, concentrated central bulge that appears yellowish-orange in color, suggesting an older stellar population and a relative paucity of ongoing star formation in that region. Diffuse, fainter material extends outwards from the bulge, forming a less defined disk. The disk exhibits a subtle color gradient, with bluer hues towards the outer edges, which may indicate the presence of younger stars or ongoing star formation in these peripheral regions. There is some visual indication of minor disturbance of the galaxy's structure.
