The galaxy presents a largely elliptical morphology, appearing predominantly smooth and spheroid in shape. The light distribution is concentrated towards the center, indicating a prominent bulge. The galaxy's color appears to be trending towards redder hues, suggesting an older stellar population and low current star formation activity. No prominent spiral arm structures or dust lanes are visible, nor any obvious signs of tidal disturbance or ongoing major merger activity. There is a slight elongation visible, deviating from a perfectly circular shape. This could be from a minor merger. Overall, the galaxy appears to be a relatively quiescent and evolved system.
