The galaxy appears to be a relatively smooth, centralized object. Its color profile suggests a population of older stars, possibly with ongoing, but low levels of star formation. The overall shape is approximately round, showing neither a prominent disk structure nor significant elongation. There is some subtle irregularity in the galaxy's outskirts, with no strong evidence of major mergers or significant tidal disturbances. The central region is brighter than the surrounding areas, suggesting a concentration of stellar mass. Based on its appearance, it may be an early-type galaxy, such as an elliptical or lenticular, at an approximate distance of 158 mega parsecs.