The galaxy presents as a generally smooth and centrally concentrated object. The core region exhibits a yellowish-white hue, suggestive of an older stellar population and lower ongoing star formation activity. The outer regions of the galaxy appear bluer, hinting at the presence of younger, hotter stars, potentially indicating recent or ongoing star formation processes in these areas. The galaxy appears somewhat elliptical in shape, deviating slightly from a perfect sphere. There is little evidence of a prominent disk structure or spiral arms. There is a faint, subtle asymmetry in the outer regions. The galaxy does not appear to be undergoing a major merger, though there might be some minor disturbance or interaction influencing its shape. Overall, the galaxy presents as a relatively evolved system, potentially transitioning towards a quiescent state.
