The galaxy presents as a largely smooth, elliptical-like structure. It exhibits a cigar-shaped morphology, noticeably elongated rather than perfectly spherical. The light profile appears to be concentrated towards the center, suggesting a prominent bulge. The color index indicates a redder hue, consistent with an older stellar population and suppressed star formation. There are no visually prominent spiral arms or significant dust lanes. The galaxy seems relatively undisturbed, with no obvious signs of ongoing major mergers or tidal interactions. However, subtle irregularities or minor disturbances may be present upon closer inspection of the image.
