The galaxy appears to be a relatively smooth, elliptical system. It exhibits a concentrated central bulge which gradually fades into a more diffuse halo. The overall color profile is trending towards a redder hue, suggesting an older stellar population. While there is no clear, active star-forming region apparent, faint blue-ish tinges indicate that there could be very low levels of recent star formation. There are no obvious signs of spiral arms or a well-defined disk structure. The galaxy shows no visible signs of any major mergers or tidal disturbances, such as streams or shells, though the low resolution makes it difficult to rule out minor interactions. The galaxy is mostly round. 
