The galaxy presents as a primarily smooth, elliptical-like structure. A central concentration of light is observed, suggesting a bulge or core region. The overall color appears yellowish-white, with subtle hints of green near the center. This color profile could be indicative of a relatively older stellar population and a lower rate of ongoing star formation. The galaxy seems fairly isolated with no apparent major mergers occurring, although a minor disturbance within the galaxy can't be ruled out from this image alone. The morphology leans towards a rounded shape, with minimal elongation detected.
