The galaxy presents as a relatively smooth, elliptical-like structure with a bright central bulge. The core appears more yellow/orange, suggesting an older stellar population. The outer regions exhibit a bluer hue, hinting at more recent star formation, though this is not pronounced. The galaxy's shape is largely in between round and oblong, with no pronounced spiral arm structures visible. There is no clear evidence of a major ongoing merger, though there may be signs of minor disturbances in the overall light distribution. The galaxy appears relatively isolated, without any obvious large companions or signs of strong tidal interactions. The approximate physical size appears to be moderately large.
