The galaxy presents as a relatively smooth, centrally concentrated object, likely an elliptical or S0 type galaxy. It exhibits a slight elongation, approaching a round shape, with no distinct spiral arms or bar structures visible. A bright central bulge is evident, gradually fading into an extended halo. The galaxy displays a subtle blue hue, suggesting a moderate amount of recent star formation, although not at a high rate. There may be evidence of a minor tidal disturbance in the form of faint asymmetry. The color index (G-R and R-Z) suggests an intermediate stellar population, with ongoing or recent star formation. Given its smooth appearance, it does not appear to be undergoing a major merging event, but there could be minor disturbances.
