The galaxy presents a primarily smooth and rounded morphology, with a slightly elliptical shape. The central region exhibits a distinct reddish hue, suggesting an older stellar population and/or significant dust obscuration. Moving outward from the core, the color shifts toward a greenish-yellow, potentially indicating the presence of younger stars and ongoing star formation in the outer regions of the galaxy. There is no clear evidence of spiral arms or a prominent disk structure. No significant tidal features or major disturbances are visible, although there may be some minor irregularities in the outer envelope. Overall, the galaxy appears to be relatively isolated and well-defined, with no obvious signs of a recent major merger.
