The galaxy presents a largely smooth morphology. The object exhibits a pronounced central bulge with a bright, concentrated core, suggesting a high stellar density in this region. The galaxy appears to be relatively round with a mostly featureless disc, indicating an elliptical or S0 type classification. There is a slight suggestion of asymmetry or disturbance in the outer regions, hinting at a possible past or ongoing interaction or minor merger event. The color profile indicates a redder hue, implying an older stellar population and a relatively low star formation rate.
