The galaxy presents a generally smooth morphology, with an elliptical shape appearing somewhere between round and mildly elongated. It exhibits a bright, concentrated central bulge that appears yellowish, indicating a population of older stars. Moving outward from the center, a subtle color gradient is observed, transitioning to a slightly bluer hue in the outer regions, possibly hinting at ongoing, albeit subdued, star formation activity. There are no distinct spiral arms or features indicative of a recent major merger event, and it does not appear to be significantly disturbed. The overall structure suggests a relatively evolved system, likely a disk galaxy, viewed at an angle.
