The galaxy presents an elliptical morphology, appearing largely smooth in structure with a dominant central bulge. The light distribution is concentrated towards the center, gradually decreasing outwards. There's a slight elongation in its shape, leaning towards a more oblate spheroidal form rather than perfectly circular. Color gradients suggest a redder core region likely populated by older stellar populations. The galaxy does not display any prominent spiral arms, dust lanes, or signs of recent major mergers, though the very slight blueness outside the core may indicate limited star formation. The galaxy is relatively isolated, showing no signs of tidal interactions with neighboring galaxies.
