The galaxy presents as a relatively smooth, elliptical-like object with a concentrated central bulge. There are no visible spiral arm structures or dust lanes discernible in the image, suggesting a more evolved system. The galaxy displays a yellowish-red hue, indicative of an older stellar population and potentially lower levels of ongoing star formation. It appears to be somewhat isolated, with no immediate signs of major interactions or mergers, although a possible minor disturbance or interaction cannot be ruled out due to slight asymmetries in its outer regions. The object's apparent roundness suggests a roughly spheroidal morphology.
