The galaxy presents as a somewhat elliptical system with a notable central bulge. The bulge exhibits a smooth, concentrated light profile, suggesting a relatively old stellar population dominating this region. The disk surrounding the bulge displays a bluer hue, indicative of more recent star formation activity, although the distribution appears relatively smooth and lacks prominent spiral arm structures. Overall, the galaxy appears to be an intermediate spiral or lenticular galaxy viewed at a slight inclination. There are faint irregularities or disturbances in the outer regions of the disk suggesting possible interaction or past merger events. 
