The galaxy presents as a smooth, elliptical structure with a concentrated central bulge. It exhibits a yellowish-orange hue, suggesting a population of older stars. There appears to be some minor evidence of disk-like structures or faint arms, but they lack definition and are not prominent. The galaxy appears isolated, with only some minor tidal disturbance apparent. There may be a minor interaction or recent merger event. Overall, the galaxy exhibits characteristics of a relatively massive system with low star formation activity.
