The galaxy appears as a centrally concentrated object, with a smooth, elliptical morphology. The core region presents a yellowish hue, suggesting an older stellar population with less ongoing star formation. Moving outward, the light distribution gradually fades, with a subtle shift towards redder colors, possibly due to dust obscuration or a change in the average stellar age within the outer regions. There is no clear evidence of spiral arms or a distinct disk component. Some minor asymmetric or irregular features are observed, possibly indicating tidal disturbances or recent minor mergers.
