The galaxy presents as a centrally concentrated object with a generally smooth morphology. It exhibits a slightly elliptical shape. The core region is a bright, yellowish-orange hue, suggesting an older stellar population. Moving outward from the center, the galaxy appears to fade gradually into a more diffuse halo. Some subtle, bluer components are visible in the outer regions, potentially indicating areas of ongoing, but limited, star formation. There appears to be no strong evidence of a prominent disk structure or ongoing major merger activity, though subtle features are visible. The galaxy does not appear to be perfectly rounded, leaning towards a slightly elongated form.
