The galaxy presents as an elliptical morphology, appearing largely smooth with a high degree of central concentration. The object exhibits a color gradient, transitioning from a yellowish-orange core to a more reddish-orange periphery, indicative of an aging stellar population. The galaxy's shape is more in-between rather than perfectly round, nor cigar shaped. There's slight evidence of minor disturbances that suggest possible interactions or minor merging events in the past. Based on the colors, star formation appears to be suppressed.
