The galaxy presents as a centrally concentrated object, with a smooth, diffuse light profile. There is a notable lack of distinct spiral arm structures or prominent dust lanes. The central bulge exhibits a bright, concentrated glow, transitioning outward to a fainter, less defined disk. The overall color appears to be somewhat red, suggesting an older stellar population and a relatively low rate of on-going star formation. There may be very minor disturbances or irregularities in the outer regions, but these are not prominent enough to suggest an ongoing or recent major merger event. The galaxy's shape is generally elliptical.
