This galaxy presents as an elliptical type, although with slight disturbances in its morphology. The central bulge region exhibits a concentrated, yellow hue suggesting a population of older stars. Moving outward from the core, a fainter, bluish halo is visible, indicative of some younger, hotter stars and possibly ongoing star formation. There appear to be very slight tidal features extending from the main body, potentially hinting at a minor interaction or merger event in its past. Overall, it appears to be a fairly massive system undergoing a transition phase, possibly migrating from a more actively star-forming state to a more quiescent one.
