The galaxy appears as a relatively smooth, lenticular-like structure with a central bulge. There is a hint of a disk, though it lacks distinct spiral arms. The galaxy is not perfectly circular; it is somewhat elongated, though not extremely so. There are no signs of ongoing major mergers or strong tidal disturbances, though there may be minor disturbances that are very difficult to detect. The galaxy exhibits a fairly consistent color profile, with a dominant reddish hue, suggesting an older stellar population and a relatively low star formation rate.
